The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated luminosity profile. It presents an overall yellowish hue, suggestive of an older stellar population. There is a slight elongation, indicating a deviation from a perfectly spherical shape. No distinct spiral arms or prominent dust lanes are discernible within the resolution afforded by the image. Indications of minor tidal disturbances or interactions are potentially present but not definitively confirmed; there is a subtle asymmetry in the outer regions of the galaxy that may or may not be the result of interaction with another celestial object.
