The galaxy presents as an elliptical or lenticular type. The light distribution is relatively smooth and centrally concentrated, with a noticeable falloff in intensity toward the outer regions. There is little evidence of spiral arm structure or distinct dust lanes. The overall shape is somewhat elliptical. There appears to be a slight deviation from perfect circularity, but not a highly elongated form. No significant tidal features or signs of a recent major merger are observed, although a subtle asymmetry or minor disturbance cannot be entirely ruled out. The galaxy exhibits a moderate color, leaning towards the redder end of the spectrum, indicative of an older stellar population.
