This galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical. The overall color profile suggests a dominant population of older stars, contributing to the observed redder hues. There is a subtle disk component. No major disturbances are detected, though there is a suggestion of a minor tidal interaction. The star formation rate is low, and the specific star formation rate is similarly suppressed, indicative of a quiescent galaxy nearing the red sequence. The galaxy appears largely undisturbed, with a classification of 0.78, indicating the galaxy appears smooth. The radius is roughly 3.4 kiloparsecs.
