The galaxy presents as a single, luminous spheroid. Its core exhibits a concentrated, bright yellow color, suggesting a significant population of older stars. There are hints of redder regions in its outer areas, which may be related to dust or the aging of the star population. The galaxy appears mostly undisturbed, lacking clear tidal features or other signs of ongoing mergers. It looks like a very relaxed galaxy, with no signs of high star formation. The general color information suggests a evolved stellar population with old stars that are not forming new stars at high rates. The galaxy's morphology is smooth and rounded, suggesting a relatively old and dynamically settled structure. There is no evidence of a prominent disk or spiral arms.
