The galaxy appears to be a relatively bright, elongated system, presenting an edge-on or highly inclined disk. A prominent bulge is observed, exhibiting a yellowish hue, suggestive of an older stellar population. The disk itself appears somewhat smooth and featureless, lacking distinct spiral arm structures or prominent dust lanes in this image. The overall color gradient transitions from the yellowish central bulge to a bluer periphery, potentially indicating younger stars in the outer regions. There is a faint, blue object in the lower part of the image, which could either be a foreground object or an area of star formation within the galaxy. There is no visual evidence of ongoing major mergers or significant tidal disturbances. The galaxy appears to be a relatively isolated system, based on the lack of nearby interacting galaxies.
