The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth luminosity profile. The core exhibits a high surface brightness, suggesting a dense stellar population. The morphology is dominated by a spheroidal component with little evidence of spiral arms or prominent disk features. The isophotes appear relatively smooth and concentric, with a slight elongation. The color gradient indicates a population of older stars. There is limited evidence of dust lanes or patchy star formation. The overall appearance is consistent with a galaxy undergoing minimal star formation. The galaxy does not appear to be undergoing any major mergers but does show hints of a minor disturbance. The image data is consistent with a galaxy whose shape falls somewhere between perfectly round and cigar shaped, leaning more toward round.
