The galaxy presents as an elongated, ellipsoidal structure, with a central bulge that appears quite prominent. The color profile suggests an older stellar population dominating the central region, indicated by the yellowish-orange hue. Moving outward from the center, a subtle disk-like structure is observable, displaying a bluer tint. This suggests the presence of younger, hotter stars and ongoing star formation, albeit at a seemingly modest rate. The smooth appearance of the galaxy indicates it is likely an early type spiral or lenticular galaxy with a dominant smooth component, with little evidence of significant dust lanes or spiral arm structures. There may be some evidence of minor disturbances in its shape. The overall morphology leans toward a cigar shape. There are no signs of major mergers or tidal interactions occurring.
