The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a bright, compact core that diffuses outward into a more tenuous halo. There is no apparent disk structure, spiral arms, or significant dust lane obscuration visible. The galaxy appears somewhat round in shape, lacking any significant elongation or cigar-like morphology. There is no evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy. The color profile suggests a population of older stars, with the overall light tending towards redder wavelengths. The galaxy shows signs of moderate ongoing star formation.
