The galaxy appears to be a luminous elliptical or lenticular type, exhibiting a smooth, centrally concentrated morphology. It is elongated in shape, with a moderate ellipticity, not appearing particularly circular or cigar-shaped. The light distribution is concentrated toward the center, with a gradual decline in surface brightness towards the outer regions. There is little evidence of distinct spiral arms or prominent dust lanes, suggesting a relatively old stellar population. The color profile is relatively uniform throughout the galaxy, with a slight bluer tint at the outer edges, suggestive of more recent, but weak star formation, and a central region that tends towards the redder end of the spectrum. There is no visible evidence of any significant tidal disturbances, mergers, or interactions with other galaxies in its immediate vicinity.
