The galaxy appears to be a relatively bright, elliptical galaxy, exhibiting a smooth, rounded morphology. Its light profile suggests a concentrated central bulge, with a gradual decline in luminosity moving outward. The galaxy displays a yellow/red hue, indicative of an older stellar population and minimal ongoing star formation. There is no visible evidence of spiral arms or a prominent disk structure. The overall form suggests a system that has largely completed its merger history and is currently undergoing a period of quiescence. There are no readily apparent signs of significant tidal disturbances or interactions with other galaxies.
