The galaxy presents as a spiral type, with a redshift of approximately 0.16. A prominent central bulge appears a yellowish-orange hue, indicative of an older stellar population. Spiral arms extend outward from the bulge, displaying a bluer tint which may suggest regions of ongoing star formation. The spiral arms appear to exhibit a grand design, with two dominant arms readily discernible. The winding of these arms is moderately open. A bar-like structure may be present, extending through the central bulge, though its definition is somewhat ambiguous. The galaxy's disk is the dominant feature. Evidence suggests a possible minor interaction or disturbance is occurring within the galaxy, as indicated by a slight asymmetry in the distribution of light in the outer disk and the irregularity of the spiral arms. The overall size appears to be relatively large.
