The galaxy exhibits a generally elliptical morphology, appearing somewhat elongated rather than perfectly spherical. Its color profile indicates a significant population of older stars, contributing to its yellowish-orange hue. There is evidence of potential interaction or tidal disruption, indicated by the presence of a brighter, redder region distinct from the main galactic body. This may be indicative of on-going merger activity. There is no clear evidence of spiral arm structure or significant dust lanes visible in this image. The galaxy appears to be of substantial mass, indicating a well-established stellar population and a likely supermassive black hole at its center. Star formation activity is observed, although is likely at a moderate rate, considering the lack of strong blue color gradients.
