The galaxy presents a centrally concentrated luminosity profile, appearing largely smooth but with possible irregularities in the distribution of light. It is dominated by a bright central region that suggests a bulge. There is a more diffuse and fainter halo of material surrounding the core, indicating a possible extended stellar population. 

The galaxy exhibits a slight deviation from perfect elliptical symmetry, with a hint of elongation in one direction. The color gradient across the galaxy is subtle, possibly indicating a variation in stellar populations with age or metallicity. In one side of the galaxy there is a distinctive color possibly indicating a separate population of stars. The overall morphology suggests a classification of either an early-type spiral or an elliptical galaxy undergoing minor interaction with another galactic body.