The galaxy presents an elliptical morphology, with a smooth, concentrated central bulge that transitions into a more diffuse outer region. The color gradient indicates an older stellar population dominating the core, emitting primarily in the redder wavelengths, while the outer regions exhibit a slightly bluer hue, suggesting the presence of younger stars or ongoing, albeit moderate, star formation. The galaxy's shape is generally round, with a slight elongation. There's no obvious evidence of significant tidal disturbances, major mergers, or pronounced spiral arm structures. However, subtle irregularities in the outer envelope might suggest minor interactions or past accretion events. Overall, it appears to be a relatively undisturbed, moderately massive system.
