The galaxy exhibits a primarily smooth morphology with a bright, concentrated central bulge. The overall shape appears approximately round.  There is evidence of possible minor tidal disturbance or interaction in the form of faint, asymmetric extensions or irregularities extending from the main body, suggesting a potential merger history.  Color gradients suggest a relatively older stellar population, with the bulge exhibiting a yellowish-red hue, transitioning to slightly bluer colors in the outer regions.  However, there are also faint redder regions scattered throughout the galaxy.  There may be some evidence of a very faint disk structure, but this is not definitively clear from the image. The galaxy is moderately luminous and relatively massive. The star formation rate seems to be relatively low.
