The galaxy presents a somewhat smooth morphology, appearing elongated or cigar-shaped. There is a hint of a disk-like structure, although the overall impression is of a galaxy with a significant spheroidal component. The central region is more luminous and exhibits a yellowish or golden hue, possibly indicative of an older stellar population or dust obscuration. Fainter, bluer regions can be observed extending along the edges, potentially indicating the presence of younger stars and star formation in these areas. There is no apparent sign of a major merger or significant tidal disturbances.
