The galaxy presents as a relatively compact, elliptical-like object, exhibiting a generally smooth morphology. A bright, concentrated central region is apparent, suggesting a significant stellar density. The object's color appears to be relatively uniform, with a subtle yellow to golden hue in the central regions, which transitions to a slightly greener tint towards the outer edges. This variation could be due to varying stellar populations. There is no strong evidence of spiral arms or significant dust lanes. Minor irregularities on the edge of the galaxy suggest very small disturbances but likely no current merging activity. The smooth, symmetrical shape and concentrated central brightness indicate a relatively evolved system, likely dominated by an older stellar population with suppressed current star formation.
