The galaxy presents as an elliptical or lenticular type with a smooth, centrally concentrated light distribution. The object exhibits a reddish hue, suggestive of an older stellar population with lower rates of on-going star formation. The galaxy is elongated, appearing cigar-shaped. There is no strong evidence of spiral arms or a prominent disk structure. Faint features are present which may indicate a minor disturbance. The object does not appear to be undergoing a major merger event, nor does it exhibit features indicative of significant tidal disruption.
