The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge that gradually diffuses outward. The core is luminous and appears slightly elongated, displaying a yellow-orange hue, suggestive of an older stellar population. There's little evidence of spiral arm structures or prominent dust lanes. The outer regions fade softly into the background, hinting at a lack of active star formation in the extended halo. The galaxy presents a moderately rounded morphology, without any major distortions or tidal features indicating recent mergers or significant gravitational disturbances. Overall, the galaxy seems to be a mature system, dominated by evolved stars.
