The galaxy presents a generally smooth and rounded morphology. The central region displays a concentrated, bright core, exhibiting a yellowish hue, possibly indicative of an older stellar population. A faint, greenish-blue halo surrounds the core, extending outwards in an elliptical shape. This halo suggests the presence of a younger, star-forming population within the galaxy's outer regions. There are no readily apparent spiral arms or bar structures. The galaxy exhibits a slight elongation, deviating marginally from a perfectly circular form. No signs of major mergers or significant tidal disturbances are observed. The galaxy seems to be a relatively undisturbed system.
