This galaxy presents a somewhat elliptical morphology, though it is not perfectly spherical. A dominant central bulge region displays a yellowish hue, suggesting an older stellar population. Fainter, bluer light extends outwards from the central region, indicating possible disk structures and ongoing, though not exceptionally vigorous, star formation activity. There is some indication of minor tidal disturbances or interactions, as the outer edges appear slightly irregular. No clear spiral arm structures are discernible in the image. The overall shape suggests a system undergoing, or having recently undergone, a merger or interaction. The galaxy appears to be of intermediate mass.