The galaxy presents an elliptical morphology, exhibiting a generally smooth appearance with a central concentration of light. The radial light profile suggests a gradual decline in brightness from the core outwards. The shape is somewhat elongated. There may be a faint disk present within the galaxy. No signs of significant tidal disturbances or ongoing mergers are apparent in this image. The galaxy shows signs of ongoing star formation activity. The overall color suggests a stellar population consisting of both younger and older stars.
