The observed galaxy presents as a relatively compact and smooth object. Its overall shape approximates a circular morphology, exhibiting minimal elongation. There is no discernible spiral arm structure or distinct features indicative of a disk component. The galaxy appears to be a single, cohesive unit, showing no signs of ongoing or recent major mergers or tidal disturbances. A slight color gradient is observed, with a tendency toward a reddish hue in the galactic core, implying an older stellar population in the central region, and a bluer tinge as one moves out from the center.
