The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The light distribution is concentrated towards the center, suggesting a prominent bulge component. The core exhibits a yellowish hue, possibly indicating a population of older stars. Moving outward from the core, the color transitions to a slightly redder tone, which may indicate a change in stellar population or the presence of dust. There appears to be no strong evidence of active galactic nuclei activity or significant star formation, as it has a smooth apperance. The galaxy's overall shape appears somewhat rounded. There are no immediately obvious signs of a major merger event, though slight asymmetry cannot be ruled out.
