This galaxy exhibits an overall elliptical morphology. The central bulge region appears quite smooth and concentrated, displaying a yellowish hue, suggestive of an older stellar population. Extending outward from the core, the galaxy's luminosity gradually diminishes, with a noticeable transition in color toward slightly redder tones. This color gradient might indicate changes in stellar population and metallicity from the center outwards. The elongated shape is apparent, though not extremely pronounced. There seems to be a minor asymmetry, possibly indicative of past interactions or internal dynamics. The apparent smoothness indicates a lack of significant recent major mergers or active star formation regions.
