The galaxy presents a generally smooth morphology, with a dominant spheroid component. The shape appears to be in between round and elliptical. A faint disk may be present, but the smoothness suggests a dominant bulge. The galaxy exhibits a yellowish-orange hue, indicative of an older stellar population. No distinct spiral arms or bars are discernible. Some minor disturbances are visible. There are signs of tidal interactions with possible merging activity, indicating a complex gravitational interaction. The galaxy is of substantial size, appearing relatively luminous. Star formation activity appears to be low, based on the color and overall smoothness.
