The galaxy presents as a luminous, centrally concentrated object. Its overall morphology appears relatively smooth, lacking prominent spiral arms or strong dust lanes. The central region exhibits a bright, yellowish hue, suggesting an older stellar population. Moving outward from the core, the color gradually shifts toward a redder tone in the galaxy's halo, which might indicate a lower concentration of younger, bluer stars in the outer regions. There appears to be a slight elongation, with the shape being somewhere between round and cigar-shaped. Faint irregularities or minor disturbances in the surrounding halo are present. They may be indicative of past interactions or accretion events.
