The galaxy presents as an elliptical or lenticular type, displaying a smooth, centrally concentrated luminosity profile. The overall shape is elongated, approximating a cigar-like form. A noticeable central bulge dominates the structure, characterized by a bright, yellowish-white hue suggesting an older stellar population. Fainter, bluer light emanates from the outer regions, possibly indicating some recent, albeit limited, star formation activity. No distinct spiral arm structure or significant dust lanes are readily apparent. There is no obvious presence of major disturbances from galactic mergers.
