The galaxy presents a relatively smooth, concentrated morphology, appearing somewhat elliptical in shape. There is a central bulge exhibiting a yellowish hue, suggesting an older stellar population. A faint, disk-like structure is possibly present around the bulge, indicated by a subtle extension of light. There is an apparent slight disturbance or asymmetry visible in the galaxy's form, however the overall appearance is largely undisturbed and not undergoing a major merger event. The overall colour profile points towards a moderate level of star formation, consistent with an intermediate spiral or early-type galaxy.
