This galaxy presents as a centrally concentrated object with a roughly elliptical morphology. The central region exhibits a bright, yellowish hue, indicative of an older stellar population and potentially lower levels of ongoing star formation. Moving outwards from the core, the light gradually fades into redder tones, suggesting the presence of either dust extinction or a transition in the dominant stellar populations. There is faint evidence of a disk-like structure but it lacks well-defined spiral arms or prominent star-forming regions, and shows signs of disturbances. The galaxy is relatively smooth in appearance, lacking significant irregular features or tidal tails, but shows the appearance of an ongoing or previous merger. Overall, this galaxy appears to be a moderately massive galaxy undergoing some merger activity and likely transitioning towards a more quiescent state.
