The galaxy presents as a somewhat elongated, smooth object with a concentrated central bulge. The color distribution suggests a population of older stars dominating the core region, appearing yellowish-orange. The outer regions show a bluer hue, hinting at the presence of younger stars, and possibly ongoing, though perhaps subdued, star formation. The overall shape is somewhat irregular, with a hint of a possible tidal feature or minor disturbance on one side. No distinct spiral arm structure is visible. The galaxy does not appear to be undergoing a major merger, but a possible minor interaction or internal disturbance is not out of the question. The galaxy appears to be of intermediate size and mass.
