The galaxy appears as a relatively smooth, elliptical-shaped object. Its core exhibits a concentrated luminosity gradient, transitioning to a slightly fainter, diffused halo. The color profile suggests a predominantly older stellar population with a subtle indication of ongoing, albeit low, star formation as indicated by the slight blue-green hue present in the outer regions. There is no obvious evidence of a prominent disk structure, spiral arms, or significant tidal distortions. Based on its morphology, this galaxy likely evolved through a period of active star formation, resulting in its redder color, and settled into a quiescent state.
