The galaxy presents as a single system with a relatively smooth, amorphous structure, showing little evidence of spiral arms or a defined disk component. The morphology appears generally elliptical, tending toward a cigar shape rather than perfectly round. The galaxy exhibits a yellow-red color gradient centrally, indicating a population of older stars. There seems to be evidence of some disturbance or interaction, potentially a merger in progress, given the system's slightly irregular shape and a small blue-ish tinged region. There is no clear evidence of active star formation within the primary body of the galaxy, the image is consistent with a population dominated by older, less massive stars.
