The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, which appears yellowish, suggesting an older stellar population. The galaxy's light profile transitions from a bright core to a more diffuse outer halo. The isophotes show a moderate degree of ellipticity, indicating it is somewhat elongated. There is some indication of a slight disturbance in the overall symmetry, perhaps hinting at a minor interaction. Faint, diffuse arms may be present, but the image resolution limits definitive identification. The overall color suggests a mix of stellar populations, with older stars concentrated in the bulge and potentially younger stars in the outer regions. The apparent size is relatively small, indicating a considerable distance.
