The observed galaxy presents as an elliptical or lenticular system, exhibiting a relatively smooth, centralized light distribution. The galaxy is elongated, but not markedly so, with an intermediate axis ratio. There is no prominent disk structure visible. The color profile is generally redder than the background sky, indicating a population dominated by older stars and/or a significant dust component. No obvious spiral arms or features of active star formation are apparent upon visual inspection. There is some indication of a minor disturbance and the possibility of an ongoing or past merger event, but it is not heavily distorted.
