The galaxy presents a generally smooth, elliptical morphology. There's a high degree of radial symmetry, with a concentrated central bulge that dominates the light profile. Faint extensions can be observed with a cigar shape. The galaxy appears yellowish-orange overall, suggesting a dominant population of older stars and a relatively low rate of ongoing star formation. There is no visible evidence of spiral arms, distinct dust lanes, or significant star-forming regions. The galaxy does not exhibit any strong tidal features or morphological disturbances, indicating it's likely not undergoing a major merger, although some minor disturbances cannot be ruled out.
