The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy. It exhibits an elongated, cigar-like shape. The central region appears to be a bright yellowish-white, suggesting a population of older stars. The outer regions of the galaxy display a bluer hue, hinting at the presence of a younger stellar population, although the overall star formation rate seems to be quite low. No distinct spiral arm structure or significant dust lanes are visible. There is no clear evidence of a major ongoing merger. A slight irregularity on the edge of the galaxy could suggest a minor interaction or tidal disturbance, but this feature is not pronounced. Overall, the galaxy appears to be a mature, quiescent system.
