The galaxy appears to be an elliptical galaxy, characterized by a largely featureless, smooth morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region residing at the core. There is a decrease in luminosity as radial distance increases, fading into the background. The color profile suggests an older stellar population with a slightly yellow hue. The isophotes are generally round, indicating a relatively relaxed system. There is no discernible dust lane or spiral arm structure visible. There may be some minor asymmetries in the outer regions. The galaxy seems to be relatively isolated. There is no obvious evidence of any major ongoing merger activity or strong tidal interactions.
