The galaxy exhibits a roughly elliptical morphology, appearing primarily smooth with a highly concentrated central region. The light profile suggests a gradual decrease in intensity moving outwards from the core. There is a suggestion of disturbance within the system. It appears to be undergoing minor distortions, which can be observed as faint deviations from a perfect elliptical shape. These features are consistent with early stage galaxy mergers.

The color indices indicate a broad spectral energy distribution. In particular, the central region shows a strong blue component, implying a population of hotter and likely younger stars. Redder colors are detectable as one moves further from the galaxy's center, which could be indicative of a population of cooler, older stars, or of the presence of dust. The overall light distribution reveals a possible interaction or merging event with faint extensions of lower surface brightness surrounding the primary structure.
