The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. The central region is bright and concentrated, suggesting a substantial stellar population and potentially an active galactic nucleus. There is a slight elongation but it maintains a mostly spheroidal shape. A faint, diffuse halo surrounds the bright core, indicating a gradual decrease in stellar density with increasing radial distance. The color distribution appears fairly uniform across the galaxy, with a tendency toward slightly redder hues, characteristic of older stellar populations. There is a potential merging event or minor disturbance and some irregularity in the outer regions, suggesting past or ongoing interactions with another galaxy or dwarf galaxy. Based on the overall appearance, the galaxy is likely a massive system with a relatively low rate of ongoing star formation.
