This galaxy exhibits a predominantly smooth morphology, with a subtle disk-like structure possibly present. The central region displays a bright, concentrated luminosity, suggesting a substantial stellar population within the bulge. The overall shape is moderately elliptical, deviating slightly from a perfect circle. There's a hint of a minor asymmetry or disturbance in the outer regions, possibly indicative of a past minor merger event. The galaxy displays a color gradient, transitioning from a yellower core to slightly bluer outer regions, potentially reflecting variations in stellar ages or metallicity. Star formation is likely occurring, albeit at a relatively low rate. The galaxy appears relatively isolated, with no obvious signs of ongoing major mergers or interactions.
