The galaxy presents as a relatively compact, elliptical morphology. The light profile appears smooth and centrally concentrated with a slight elongation. The galaxy exhibits a color gradient, transitioning from a yellowish core to a redder halo. There is no discernable spiral arm structure or obvious dust lanes. The galaxy's overall structure suggests a lack of significant recent merger events. Star formation appears suppressed, based on the redder color, implying a population of older stars dominate. There is no visual evidence of active galactic nuclei activity from this image. The size of the galaxy is moderate.
