The galaxy presents as an elliptical or lenticular type, characterized by a smooth, diffuse light distribution without prominent spiral arms. The central bulge appears relatively bright and concentrated, gradually fading into the outer regions. There is little evidence of significant dust lanes or active star formation within the visible spectrum. The overall shape is somewhat elongated, suggesting a possible deviation from a perfect spherical symmetry. No apparent major merging activity or tidal features are detected. The galaxy exhibits a blueish central hue, which becomes more reddish towards the outskirts, suggesting a difference in stellar populations. The galaxy appears to be relatively isolated.
