The galaxy presents a largely smooth morphology, exhibiting a concentrated central bulge that diffuses outward into a fainter, less defined disc structure. The color profile suggests a population of older stars, with a dominant yellowish-red hue, particularly concentrated in the core. There is little evidence of significant recent star formation within the visible spectrum. The galaxy appears somewhat elliptical, leaning towards a more circular shape, rather than being highly elongated. There are some slight indications of minor gravitational interactions or internal disturbances, although the dominant impression is one of relative quiescence and established structure. Any potential tidal features or disrupted morphologies are subtle, contributing to the generally smooth appearance.
