The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth, concentrated morphology with minimal discernible spiral arm structure. The central bulge dominates the overall light profile, appearing bright and slightly yellow in color, suggestive of an older stellar population. The galaxy appears to be relatively isolated, showing no prominent signs of ongoing major mergers or tidal disturbances. The morphology is primarily smooth, with a nearly round appearance, suggesting a high degree of internal order and stability. Faint irregular extensions on its edges may indicate past or minor interactions. The low presence of blue light suggests a lack of recent, major star formation activity within the visible region.
