The galaxy presents as an elliptical or lenticular type with a smooth, centrally concentrated luminosity profile. The core is a bright yellowish-white, indicative of an older stellar population. Fainter, diffuse light extends outwards from the core in an elongated shape, suggesting it is not perfectly spherical. There is no apparent spiral structure or dust lane visible. There might be a very slight tidal disturbance or minor interaction on the far right side of the galaxy, but it is very faint. Overall, the galaxy appears to be relatively undisturbed, with no signs of active star formation indicated by the lack of blue or patchier regions, and the dominant yellowish hue.
