This galaxy appears to be a relatively compact system, likely a spiral galaxy. Its central region displays a high degree of luminosity, which diminishes gradually with distance from the center. While there are some visible clumps of material, the overall impression is that the galaxy lacks well-defined spiral arms.

The galaxy's color profile suggests a mixed stellar population. The inner regions exhibit a slightly bluer hue, potentially indicating the presence of younger, hotter stars. The outer regions have a more reddish tint, suggestive of older, cooler stellar populations.

There is evidence of some kind of gravitational disturbance within the galaxy. The system’s shape deviates slightly from a perfectly smooth elliptical form. This could point toward a past interaction with another galaxy.
