The galaxy presents a generally smooth morphology, with little evidence of significant substructure or spiral arms. The light distribution appears centrally concentrated, indicative of a prominent bulge. There is a slight elongation to the galaxy's shape, appearing somewhere between round and cigar-shaped, suggesting it is elliptical. Color gradients are present, the core appears bluer than the outer regions, possibly indicative of ongoing star formation at the core. There seems to be no signs of tidal tails or distortions suggestive of any recent major merger event, although a very subtle irregularity could be interpreted as a minor disturbance. The object appears relatively isolated within its field of view.
