The galaxy presents as a relatively smooth, elliptical structure, characterized by a dominant, concentrated bulge. The core region exhibits a bright, yellowish-orange hue, suggesting a population of older stars. There is a subtle extension of light outwards from the core, forming a faint halo. The overall morphology indicates a minimal disk component, with the galaxy appearing largely spheroidal. There is no clear evidence of ongoing merging activity or major tidal disturbances. The galaxy's shape is neither perfectly round nor elongated to a significant degree. Overall, the galaxy appears to be a relatively quiescent system with a red shift of 0.293170.
