The galaxy presents as a single, relatively smooth and centrally concentrated light distribution. It displays a nearly circular morphology, with only minor deviations from a perfect ellipse. There is no discernable spiral structure or bar present. The galaxy appears to be dominated by an older stellar population as evidenced by the overall reddish hue, but may possess a small degree of recent star formation. There is no evidence of any major mergers or tidal disturbances. The galaxy appears to be isolated, not part of a larger galaxy cluster. The galaxy is slightly brighter in the red bands than in the blue bands. The object appears to be a galaxy because it is slightly fuzzy and not as pinpoint as a star.
