The galaxy presents a smooth, elliptical morphology, with a concentrated central bulge that emits strongly across the observed visible spectrum. There is an apparent lack of distinct spiral arm structures or prominent dust lanes. The galaxy's overall color is slightly red-shifted, indicating a population of older stars and potentially lower ongoing star formation. While not perfectly spherical, it deviates only moderately from a circular shape, leaning towards a more oblate spheroid form. There is no visually apparent evidence of major ongoing merging activity or tidal disturbances that would strongly disrupt the overall structure. Minor irregularities in the outer regions are suggestive of the presence of a faint disk.