The galaxy presents as a centrally concentrated object with a smooth light distribution, transitioning gradually from a bright core to fainter outer regions. The morphology appears largely elliptical or lenticular, lacking distinct spiral arm structures. There is a slight elongation in its shape; it appears to be more "in between" than a perfectly round shape. The galaxy exhibits a yellowish hue in its central region, indicative of an older stellar population. The outer regions have a hint of a bluer color, and also are more irregular. There is no clear evidence of tidal tails or significant distortions, suggesting a relatively undisturbed system. However, the slight irregularity in the outer regions could hint at a minor interaction.
