The galaxy presents a largely smooth, elliptical morphology. There is a slight elongation, appearing more 'in between' a round and cigar shape rather than distinctly circular. No pronounced spiral arms or disk-like features are readily discernible. The light is concentrated towards the center, consistent with a bulge-dominated system. There is little to no evidence of active merging or major disturbances in its structure. The color profile indicates a population of older stars, with a general lack of blue emission suggesting relatively low levels of recent star formation. The object's luminosity is relatively high.
