The galaxy presents as a somewhat elliptical structure with a prominent, bright central bulge. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population and reduced star formation activity in the galactic nucleus. Fainter, diffuse blue light extends outwards from the central region, indicating the presence of younger, hotter stars within the disk, though this feature is not particularly prominent, leading to the interpretation that star formation may be relatively low. The disk is elongated, with a cigar-like appearance and some indications of minor disturbances or tidal features, perhaps from a past or ongoing interaction with another galaxy, though no companion is immediately visible. Overall, the galaxy appears relatively smooth, with no clear spiral arm structure discernible.
