The galaxy presents as a centrally concentrated, smooth elliptical system. Its morphology is dominated by a spheroidal component, with a noticeable lack of spiral arm structures. The light distribution appears relatively uniform across the galaxy, with a gradual decrease in intensity from the core outwards. The color gradient suggests a relatively old stellar population, characterized by a yellowish-red hue. No prominent dust lanes or active star-forming regions are discernible within the galaxy's disk. The galaxy exhibits a compact structure, with a well-defined boundary. There is no evidence of ongoing merging activity or significant tidal disturbances. The overall appearance suggests a relatively evolved and quiescent system, potentially a massive elliptical galaxy at intermediate redshift.
