The galaxy presents a smooth, elliptical morphology. The light distribution appears centrally concentrated, exhibiting a bright, yellowish core that gradually fades into the outer regions. The overall shape is elongated, approximating a cigar-like form. There is no obvious presence of spiral arms or a distinct disk structure. The galaxy appears relatively undisturbed, with no significant signs of ongoing mergers or tidal interactions. The color gradient suggests a population of older stars dominating the galaxy's stellar content, with a possible hint of bluer regions in the lower portion, potentially indicating more recent, although modest, star formation. The galaxy exhibits a redshift, indicating it is at a substantial cosmological distance.
