This galaxy appears as a relatively compact object with a smooth, elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes. The light distribution is centrally concentrated, suggesting an older stellar population. The galaxy exhibits a slight elongation. There is a hint of tidal disturbance or a faint feature that suggests possible interaction or recent merger, though overall the main body of the galaxy seems undisturbed. The galaxy's overall color is somewhat blue, which suggests ongoing star formation. However, given the dominant elliptical appearance, it appears that the galaxy is primarily composed of older stars. 
