The galaxy presents as a relatively compact structure. It has a dominant central bulge and a hint of a disk component, viewed at an angle. The bulge exhibits a smooth light distribution, suggesting an older stellar population. There is some indication of spiral structure or faint features in the disk, though the image resolution limits detailed morphological classification. The color profile suggests moderate star formation. The light is primarily yellow with some blue hints, indicating a mix of stellar ages, though it is dominated by older stars. There is no clear evidence of a major merger event. The overall appearance is that of a galaxy in a relatively quiescent state of evolution.
