The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated light distribution. The core is bright and somewhat diffuse, suggesting a high concentration of stars and potentially an active galactic nucleus. The overall shape is somewhat elongated, showing a slight deviation from a perfectly spherical morphology. There is little evidence of spiral arms or significant dust lanes. The color profile suggests a population of older stars, with a lack of distinct blue regions indicative of recent star formation. There are minor irregularities in the outer regions of the galaxy, suggesting that it may be in the process of merging with another galaxy.
