The galaxy presents a largely smooth, elliptical morphology. The central bulge exhibits a high degree of symmetry and is the most luminous region of the galaxy, appearing as a concentrated, bright yellow-white hue. There is a distinct absence of prominent spiral arm structures, suggesting a classification towards the elliptical end of the Hubble sequence. The galaxy's color suggests a moderate population of older stars, contributing to the yellowish tint in the central region, with a hint of redder stars in the outer halo. There is no visually apparent ongoing major merging activity. Minor disturbances may be present within the extended, less luminous halo, as some asymmetries are observed, although the image resolution limits definitive conclusions about possible interactions or tidal features. The galaxy appears relatively isolated within its field.
