The galaxy appears as an elliptical or lenticular structure with a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish hue, suggesting a population of older stars. There is a slight extension of bluer light which could indicate a recent interaction or minor merger. The overall form is relatively undisturbed, with minimal evidence of strong tidal features or active star formation beyond the possible interaction. The size is difficult to precisely estimate due to the image resolution but it appears moderately large.