The galaxy appears as a relatively small, well-defined elliptical galaxy, exhibiting a smooth, spheroidal morphology. The galaxy's light profile appears concentrated, with a bright central bulge that gradually fades toward the outer regions. There is no apparent spiral structure or prominent disk features visible. The galaxy exhibits a yellow/white hue, suggesting a relatively older stellar population with less ongoing star formation. No significant tidal features or evidence of recent major mergers are immediately apparent, although there might be a very slight disturbance in the morphology, implying possible past interaction. The roundness of the galaxy is quite high.
