The galaxy presents as a somewhat elliptical, smooth structure. It exhibits a concentrated central bulge region that appears more luminous than its outer regions. The color gradient suggests a relatively homogenous stellar population, with a possible concentration of older stars in the central bulge. The outer regions display a bluer hue, hinting at the potential presence of younger, hotter stars and perhaps ongoing, albeit subdued, star formation. The galaxy's overall shape is somewhat elongated, with a slight deviation from a perfect spheroid. There is no immediately discernible evidence of spiral arm structure or significant dust lanes. The galaxy shows subtle signs of a minor gravitational interaction, or disturbance. Overall, the galaxy appears to be a fairly massive system.
