The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. Its morphology is largely featureless with a dominant bulge. It demonstrates a notable ellipticity, suggesting a non-spherical shape, appearing elongated or cigar-shaped. The color gradient across the galaxy indicates a relatively old stellar population, with a concentration of redder stars. There is no discernible disk structure or spiral arms. The galaxy is relatively isolated, with no major signs of tidal disturbances or ongoing mergers. Close inspection reveals some faint, disturbed features, possibly indicating a minor interaction. Overall, this galaxy presents as a passively evolving system.
