The galaxy presents as a relatively compact, elliptical-like structure with a smooth, diffused light distribution. The core region exhibits a bright, concentrated luminosity, suggesting a high stellar density. The galaxy displays a slight elongation, deviating marginally from a perfectly circular morphology. Faint hints of bluer colors are visible in the outer regions. There is some evidence of structural disturbance or interaction, as the outer edges appear somewhat irregular rather than uniformly smooth. A faint, somewhat irregular structure suggests the possibility of tidal features or minor interactions with another galaxy.