The galaxy presents as a spiral with a notable central bulge. The bulge appears moderately prominent, exhibiting a yellowish hue, suggestive of an older stellar population. Faint spiral arms extend outwards from the central region, displaying a bluer tint, potentially indicative of ongoing star formation. The overall structure is somewhat flocculent, lacking sharply defined spiral arms. There appears to be no significant bar structure bisecting the bulge. The galaxy is not observed to be edge-on, instead, it is presented at a slight angle to our line of sight. There is no apparent evidence of significant tidal disturbances or major mergers, although there is a slight asymmetry.
