The galaxy presents a smooth, elongated morphology. The central region exhibits a concentrated luminosity profile, appearing brighter and more yellow in color compared to the outer regions. The overall shape is suggestive of an elliptical galaxy viewed from an angle, possibly a prolate spheroid. There is little evidence of spiral arm structure or prominent dust lanes. The color gradient indicates a potential transition from older stellar populations in the core to potentially younger, bluer populations toward the periphery. There is no obvious sign of ongoing major merger activity or significant tidal disturbances in the immediate vicinity. The lack of distinct features such as star-forming regions suggests a relatively passive system.
