The galaxy presents as a primarily smooth, elliptical-like structure, with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. A faint, diffuse disk-like structure is subtly visible, with very little indication of spiral arms. There is only minimal evidence of ongoing star formation, and the overall color indicates a relatively quiescent state. The galaxy appears relatively isolated, with no immediate signs of major mergers or significant tidal disturbances. Its general morphology suggests a mature galaxy, possibly transitioning toward a more passive evolutionary phase.
