The galaxy presents a generally smooth morphology, appearing mostly round in shape with minimal discernible disk-like features. There is a subtle elongation, not quite cigar-shaped, but leaning away from a perfect circular form. It exhibits a yellowish-red hue, suggestive of an older stellar population and reduced levels of on-going star formation. No signs of major mergers or significant tidal disturbances are apparent from its structure, though there may be a very slight indication of minor interaction. The galaxy is relatively compact in apparent size.
