The galaxy presents a generally smooth and elliptical morphology. It exhibits a well-defined central bulge, which appears yellow-orange, indicative of an older stellar population. The outer regions of the galaxy show a bluish hue, suggesting the presence of younger, hotter stars and some ongoing star formation, though it appears to be at a modest rate. The galaxy displays a slight elongation, appearing neither perfectly spherical nor highly elongated, but rather somewhere in between. There is a suggestion of minor disturbances in the galaxy's structure, possibly due to a past or ongoing interaction with another galaxy, but no major mergers or disruptions are immediately apparent. Overall, the galaxy appears relatively undisturbed, displaying a somewhat quiescent state with a mix of old and young stellar populations.
