The galaxy presents as a centrally concentrated, slightly diffuse object. It exhibits an overall smooth morphology, with a subtle elongation suggesting a departure from perfect sphericity. There are no obvious spiral arm structures or distinct dust lanes visible in the image. The color profile appears to be relatively uniform across the galaxy, with a hint of a bluer core, potentially indicating some active star formation despite its generally quiescent appearance. There is a faint presence of tidal features that indicate a possible merger. Overall the presence of merger characteristics indicate a period of interactions.
