The galaxy presents as a fairly compact, elliptical-like object. It exhibits a smooth, largely featureless appearance. There is a slight elongation, but overall, it appears close to round. The color gradient suggests a higher concentration of younger, bluer stars in the central region, fading to slightly redder hues in the outer regions. There are no obvious signs of spiral arms or significant dust lanes. Indications suggest that this galaxy is relatively quiescent with a very low rate of star formation, representing a system dominated by an older stellar population. There are no obvious signs of tidal distortions or ongoing major merger activity, though a minor disturbance cannot be ruled out.
