This galaxy appears to be an elliptical galaxy with a generally smooth, concentrated light distribution. The primary body of the galaxy exhibits a yellowish-orange hue at its core, which may indicate an older stellar population dominating the central regions. Extending outwards from the core, the galaxy displays a slightly elongated shape, with a blueish halo enveloping it. The bluer color hints at the potential presence of younger stars, possibly from ongoing or recent star formation activity.

A potential tidal tail or companion galaxy can be seen to the right of the main body, hinting that this galaxy may be in the process of merging or has experienced a past interaction. The slight asymmetry in the overall structure further suggests a possible merger event, with some disturbance in the morphology. The galaxy seems to be a massive galaxy, with a moderate star-formation rate.
