The galaxy appears to be an elliptical, cigar shaped system exhibiting a relatively smooth morphology with a slight disk-like structure. The main body of the galaxy presents a diffuse, homogenous glow with a centrally concentrated brightness profile. It displays a pronounced elongation along its major axis. Faint extensions are detected, indicating possible tidal interactions or recent minor merging events. The colour profile suggests a population of older stars, as indicated by the redder hues at the edge of the ellipse, with some ongoing star formation concentrated in the central region, as revealed by blue colour.
