The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated, luminous core that gradually diffuses outward into a more extended halo. The overall shape is generally round, showing a minimal deviation from a spherical morphology. No distinct spiral arms or bar structures are discernible within the image. There are no obvious signs of ongoing merging activity or major tidal disturbances, and the galaxy appears relatively undisturbed. The color profile suggests an older stellar population with a yellow/red hue, possibly indicative of lower current star formation.
