The galaxy presents a primarily smooth, elliptical morphology. Its light profile is concentrated, exhibiting a high degree of central luminosity. The galaxy appears nearly round in shape, with minimal deviation towards an elongated or cigar-like form. There is no visually apparent evidence of strong tidal features, major mergers, or significant disturbances in its overall structure. The color profile suggests an older stellar population, with the light tending towards the redder end of the spectrum. This hints at a lack of ongoing, active star formation within the galaxy. The galaxy is relatively compact in size.
