The galaxy presents an overall elliptical morphology, exhibiting a smooth light distribution with no prominent spiral arm structures or bar features immediately discernible. The central region appears slightly more concentrated, suggestive of a bulge, though it lacks strong definition. The galaxy's color profile indicates a bias towards redder wavelengths, implying a population of older stars and potentially lower ongoing star formation activity. There are no obvious signs of major mergers or tidal disturbances, although subtle asymmetries or minor irregularities in the light distribution cannot be completely ruled out at this resolution. The galaxy's apparent roundness suggests a possible classification as an E3 elliptical. The light distribution appears relatively even, with no knotty star forming regions visible.
