The galaxy exhibits a primarily smooth morphology, appearing elliptical in shape, though not perfectly round. A slight elongation is observed. The central region displays high surface brightness, indicating a concentrated nucleus. Fainter, diffuse light extends outwards, gradually fading into the background sky. The color profile suggests a population of older stars. There is possible evidence of a minor disturbance or interaction, indicated by the slight asymmetry in the outer regions. The galaxy is relatively large, with a estimated size of approximately 9 kpc across, suggesting a high stellar mass. Star formation is relatively low. Analysis indicates that the galaxy might be undergoing, or have recently undergone, a merging event based on it's classification from Galaxy Zoo as a possible merger.
