The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with a bright, diffuse core that gradually fades into the surrounding halo. There is minimal evidence of spiral arm structure or distinct dust lanes. The galaxy's overall shape is generally round with no notable elongation or tidal features. The color profile suggests an older stellar population. There might be some evidence of minor disturbances present within the galaxy's structure, but it is not currently undergoing a major merger.
