The galaxy appears as a centrally concentrated object, exhibiting a roughly elliptical morphology. The central region displays a yellowish hue, potentially indicative of an older stellar population. Proceeding outwards, the color gradually shifts to a more greenish-blue, implying the presence of younger, hotter stars in the outer regions. There is subtle evidence of some disk like features, and potentially some disturbances in the outer regions. Overall, the galaxy presents an intermediate stage of evolution, showing characteristics of both a spheroidal component and a star-forming disk. There is likely a notable amount of star formation occurring within the galaxy.
