The galaxy presents as an elliptical type, with a smooth, diffuse light distribution concentrated towards a bright central bulge. A faint, flattened disk component is potentially present, but the bulge dominates the overall morphology. The galaxy's color is generally yellowish-red, suggesting an older stellar population with lower levels of current star formation. A faint blueish patch is noticeable on the outskirts of the galaxy, indicating a region of potentially ongoing, albeit minor, star formation. There is no strong evidence of spiral arm structure or a bar. No signs of major mergers are observed, although subtle asymmetries or disturbances in the light distribution may suggest minor tidal interactions or past mergers. The galaxy is moderately luminous, as indicated by its compact size and overall brightness.
