The galaxy presents a somewhat elliptical morphology, exhibiting characteristics of both a smooth, featureless spheroid and a disk component. The central bulge appears prominent, with a concentrated and relatively bright core. There is evidence of a flattened structure extending outward from the bulge, indicating the presence of a disk. The galaxy displays a color gradient, with the central regions appearing more yellow/red, suggesting an older stellar population and dust obscuration. The outer regions of the disk exhibit bluer hues, implying the presence of younger, hotter stars. There is a suggestion of minor disturbances within the galaxy's morphology, potentially indicative of past or ongoing interactions. No strong evidence for active star formation is immediately apparent in the image, although subtle color variations suggest some level of star formation activity.
