The galaxy presents as a relatively smooth, elliptical structure. A dominant, centrally concentrated bulge is clearly visible, emitting a yellowish-orange light, suggesting a population of older stars. A fainter, possibly disk-like structure extends from the central bulge, also exhibiting a yellowish hue, indicating a continuation of the aging stellar population outward. There is some evidence of a possible minor interaction or disturbance, with a less defined region towards one end. There is a clear gradient in color, and overall, the galaxy exhibits relatively little blue light, implying a low rate of ongoing star formation. The galaxy appears to be in a relatively relaxed state, with no major merger events strongly evident.
