The galaxy presents a largely smooth, elliptical morphology, with an overall round appearance and no discernible spiral arm structure. The light distribution suggests a higher concentration towards the center. The color profile appears generally yellowish-orange, possibly indicating an older stellar population with a relatively low rate of ongoing star formation. It appears as though there is a potential for a minor disturbance in the gravitational structure, though the galaxy maintains an overall undisturbed morphology. There are no prominent tidal tails or significant distortions visible. The galaxy looks like it is isolated in its environment, with no obvious signs of interactions or mergers with other large galaxies.
