The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a smooth, centrally concentrated light profile. The galaxy displays an overall yellowish-white hue, indicating a stellar population dominated by older, redder stars, which suggests that star formation is either low or has ceased altogether. There is minimal evidence of spiral arm structure or significant dust lanes. The galaxy’s shape is generally round. There seems to be a slight distortion of the galaxy's disk but not enough to classify as a major disturbance.
