The galaxy presents as a centrally concentrated, largely smooth object, exhibiting a morphology suggestive of an elliptical galaxy or a spiral galaxy seen face-on with a prominent bulge. It displays a gradual decline in luminosity from a bright, concentrated core outwards. The color profile indicates a somewhat redder core, transitioning to slightly bluer hues in the outer regions. No distinct spiral arms or dust lanes are clearly discernible within the resolution of this image, further supporting a classification leaning towards an elliptical or lenticular galaxy. There is very little evidence of any major interaction or recent merger event. Minor irregularities in the outer regions could indicate past interactions or accretion events but are not distinct enough to draw firm conclusions. Overall, the galaxy appears to be a relatively undisturbed, mature system with a moderate stellar mass.
