The galaxy appears to be a large, somewhat irregular system. It exhibits a generally smooth morphology but with some notable features that deviate from a perfectly elliptical shape. The central region is dominated by a bright, yellowish glow, potentially indicative of an older stellar population and/or dust obscuration. Surrounding the core, there is a fainter, bluer halo, particularly noticeable on one side, which could suggest regions of ongoing star formation or a younger stellar population. There is a possibility of minor gravitational interaction or disturbances within the system, hinted at by the slightly asymmetric distribution of light and some subtle irregularities in the outer regions. Overall, the galaxy is relatively luminous and appears to be a massive system.
