The observed galaxy presents as a primarily edge-on disk galaxy with an estimated diameter of approximately 3 kpc. A prominent central bulge region is observed, exhibiting a yellowish-white hue, potentially indicative of an older stellar population. Extending from the bulge, a relatively faint disk structure is visible, showing a bluer color gradient toward the outer edges. This color shift could be caused by the presence of younger, hotter stars in the disk. Irregularities in the outer disk, including faint, diffuse patches, hint at potential tidal interactions or minor disturbances affecting the galaxy's morphology. A degree of dust obscuration may be present within the disk, as suggested by darker patches or subtle variations in surface brightness. The galaxy shows an estimated redshift of 0.076, placing it at a considerable distance. Based on the red shift and magnitude, this galaxy is a very large and very bright galaxy. Based on the star formation rate, and the overall appearance, the galaxy appears to be in a transitional phase from a more active star-forming state to a more quiescent state.
