The galaxy presents a moderately elliptical morphology, with a noticeable central bulge. It exhibits a relatively smooth appearance, with little evidence of prominent spiral arms or distinct substructures. The light distribution appears centrally concentrated, with a gradual falloff in intensity towards the outer regions. The color profile suggests a population of older stars, with a predominantly yellowish-red hue, especially in the central regions. However, the presence of bluer regions suggests ongoing star formation. The outskirts appear less defined, possibly indicating a larger halo of older stars. There appears to be a mild degree of gravitational interaction happening. Some asymmetry is present, possibly a faint tidal tail.
