The galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. There is a noticeable concentration of luminosity toward the central region, suggesting a well-defined nucleus. The overall color gradient transitions from a yellowish-white core to a redder periphery. No distinct spiral arms or prominent dust lanes are discernible. The morphology suggests that it is not undergoing any major merging events, and exhibits minor disturbances if any.