The galaxy appears as a moderately luminous object with an overall smooth morphology, though potentially exhibiting some features indicative of a disk-like structure upon closer inspection. It presents a yellowish-white hue, suggesting an older stellar population is dominant. There are no distinct spiral arms or strong dust lanes readily apparent. Its shape is neither perfectly spherical nor highly elongated, appearing somewhat in-between, though closer to round. There appears to be some disturbance to the galaxy, or potentially a merger occurring, leading to some irregularity in its overall form.
