This galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light distribution. The central region exhibits a yellowish hue, potentially indicating a population of older stars. Moving outward, the galaxy transitions to a bluer color profile, suggesting a mix of stellar populations including some younger, bluer stars. There are no readily discernible spiral arms or a prominent disk structure. While the overall structure is mostly smooth, there are indications of minor disturbances, possibly due to a past interaction or minor merger. The galaxy's shape is somewhat elongated, but not excessively so, appearing to be more “in between” round and cigar shaped. Overall, it presents as a relatively quiescent system.
