The galaxy presents as a concentrated central bulge surrounded by a fainter, diffuse halo. The core exhibits a relatively smooth morphology, with a high degree of central concentration. The overall shape is generally round, though it exhibits a slight elongation. A faint arm-like or tidal feature extends away from the central region, characterized by a series of what appear to be clumps of material. The color suggests a population of older stars dominating the central bulge, with bluer, potentially younger populations present in the outer regions and the arm. The galaxy exhibits signs of possible interaction or merging activity based on the tidal extension and clumpy morphology along it. The galaxy is relatively massive and has a low rate of star formation.
