The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge that emits strongly in the red band, indicating a population of older, redder stars. The galaxy is more compact and shows no evidence of distinct spiral arms or significant disk-like structures. There is a very slight ellipticity, but overall, it appears generally rounded. There are no obvious signs of tidal tails, distorted morphology, or other major disturbances to suggest an ongoing or recent merger event, though there is a possibility of a minor interaction given slight asymmetry in outer regions. The galaxy's colour profile suggests a relatively low star formation rate and a dominant population of evolved stars.
