The galaxy exhibits a generally smooth morphology, with a predominantly elliptical appearance. The central region displays a concentrated luminosity, appearing roughly circular. A fainter, more diffuse extension is observed on one side, possibly indicative of a tidal tail or a disrupted structure due to gravitational interaction. The color distribution suggests a mix of stellar populations; the core region presents a yellowish hue, potentially indicating older stellar populations. Conversely, the fainter extension shows a bluer tint, suggestive of younger, hotter stars. There is evidence of possible merging or interaction, but it is unclear whether this interaction is in the early or late stages. The overall structure may suggest a galaxy undergoing a merger event.
