The galaxy presents as a somewhat diffuse, spheroidal object. Its overall color appears to be yellowish-red, indicative of an older stellar population with relatively low star formation activity. The light distribution is concentrated, with no apparent spiral arm structures or significant dust lanes visible. There seems to be evidence of a possible merging event. The galaxy’s morphology appears to be somewhat disrupted, displaying a non-symmetric shape which suggests a recent or ongoing interaction with a neighboring galaxy, which is supported by the blueish/purpleish object that could be the center of another galaxy.
