The galaxy presents as a single, relatively smooth, centrally concentrated light distribution. It exhibits an elliptical morphology, with a moderate ellipticity. The central region appears bright and yellowish, suggestive of a concentration of older stellar populations. Moving outward from the center, the color appears to transition towards slightly bluer hues, particularly along the major axis. These bluer regions may indicate more recent star formation activity, although the overall star formation rate appears to be low. There is no evidence of a distinct disk component or spiral arm structure. Furthermore, the galaxy does not appear to be undergoing any major merging activity or tidal disruption.
