The galaxy presents as a relatively compact, luminous object with an overall smooth appearance. The light distribution suggests an elliptical morphology, but with a slight asymmetry that could hint at possible interactions or internal structures. There is a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a more yellowish core. This may indicate ongoing, but not very vigorous, star formation in the outer parts of the galaxy, while the core appears dominated by an older stellar population. The galaxy doesn't exhibit any obvious signs of strong tidal disturbances or prominent spiral arm structures. Overall, it appears to be a galaxy of intermediate mass and star formation activity.
