The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated light profile. The central region shows a bright, yellowish-white hue, indicating an older stellar population likely dominated by red giant stars. Moving outwards, the galaxy's color shifts slightly to a less saturated yellowish-green. There is minimal evidence of spiral arms or distinct features, the light gradually fading into the background. The galaxy shows very little internal structure. There may be a slight tidal disturbance or interaction, but there is no clear evidence of a major ongoing merger event. The overall shape of the galaxy appears close to round.
