The galaxy presents as a largely featureless, smooth elliptical. There is a high degree of central concentration, with the luminosity peaking at the core and gradually fading towards the edges. The overall shape appears to be somewhat elliptical, but not significantly elongated. The light profile suggests a relatively homogenous stellar population within the galaxy, with no distinct spiral arm structures or prominent dust lanes visible. A slight color gradient is observed, with the core appearing more yellow/orange and the outer regions trending towards a bluer hue. This may indicate differing stellar populations, with older, redder stars dominating the core and a younger, bluer population in the outskirts, though this needs confirmation. There might be some subtle irregularities in the outer isophotes suggesting minor tidal interactions, but no major merging signatures are immediately apparent.
