The galaxy appears to be elliptical in morphology, with a smooth, featureless structure. It exhibits a high degree of central concentration, with the luminosity gradually decreasing towards the outer regions. The color profile suggests an older stellar population, leaning towards redder wavelengths, with the central region appearing slightly more luminous than the outer halo. There is no discernible dust lane or spiral arm structure visible. No major mergers or tidal features are apparent, suggesting it has not undergone any major interactions in recent history. The shape is generally round with a slight deviation toward being less rounded.
