The galaxy presents a generally smooth morphology, though it exhibits a somewhat elongated, cigar-shaped structure. A distinct color gradient is apparent. The core region appears to be exhibiting light on the redder end of the spectrum. This transitions towards bluer light as we move towards the outer edges of the galaxy, although a portion is obscured. This feature could be the result of varying stellar populations or dust obscuration. The galaxy does not exhibit any obvious signs of a major merger event, and the general structure points toward it being an elliptical galaxy.
