The galaxy presents as an elliptical or lenticular structure with a smooth, centrally concentrated light distribution. It exhibits a largely spheroidal morphology, with a gradual decline in luminosity moving outward from the core.  There are no apparent spiral arms or significant dust lanes visible within this system. The color profile suggests a population dominated by older stars, evidenced by the yellowish-red hue, with a small amount of ongoing star formation. There is no indication of any major ongoing merger activity, though a very minor disturbance cannot be fully ruled out. Overall the galaxy appears to be relatively isolated with no clear signs of interaction with neighboring galaxies.