The galaxy presents a largely smooth and elliptical morphology, with a concentrated central bulge. There is little to no indication of spiral arm structure or prominent dust lanes. The light distribution appears fairly uniform, decreasing gradually from the core outwards. The galaxy exhibits a yellowish-white color in its central region, transitioning to a bluer hue towards the outer edges. This color gradient could indicate a relatively older stellar population in the core and a younger, more active star-forming population in the surrounding regions, though overall star formation activity appears to be low. The overall shape appears generally round, with minimal elongation or distortion, suggesting it is likely not undergoing any major merging events or gravitational disturbances. The galaxy appears relatively isolated and undisturbed.
