The galaxy presents as an elliptical morphology. It exhibits a centrally concentrated luminosity profile with a bright, unresolved core, likely containing a supermassive black hole. The galaxy appears generally smooth with a fairly high degree of circular symmetry. No distinct spiral arm structures or bar features are discernible in this image. Faint, diffuse extensions are visible extending from the central region, suggesting the presence of a stellar halo or tidal features but no significant signs of recent or ongoing major mergers are evident. The colors within the galaxy suggest an older stellar population. The inner regions of the galaxy are slightly redder than the outer regions. Overall, the galaxy appears to be relatively isolated with no interacting companions visible in this field of view.
