The galaxy presents a moderately elongated, elliptical morphology. It exhibits a smooth, diffuse appearance, with a bright central bulge. The color profile suggests a relatively evolved stellar population, with a dominant yellowish hue in the core, indicative of older stars. There's some evidence of bluer regions on the periphery, potentially indicating areas of more recent star formation. A slight asymmetry or disturbance can be observed in the galaxy's outer regions, potentially hinting at a past or ongoing minor interaction.
