The galaxy presents an elliptical morphology, appearing mostly smooth with a high degree of central concentration. The object is somewhat rounded, though not perfectly circular, exhibiting a slight elongation. There is no discernible spiral arm structure or obvious disk component. The galaxy's color profile suggests a relatively evolved stellar population with a dominance of older, redder stars. The lack of significant blue color indicates a lower rate of on-going star formation activity. There are no signs of major mergers or tidal disturbances in its immediate vicinity, although subtle irregularities may indicate minor past interactions. Overall, this galaxy appears to be a mature, relatively quiescent system.
