The galaxy appears as a largely featureless, elliptical or lenticular structure with a smooth light distribution. Its overall color is yellowish-orange, suggesting a population of older stars with relatively little ongoing star formation. There is a slight elongation to its shape, but it largely appears rounded. No distinct spiral arms or bar structures are visible. The galaxy's light profile suggests a dense central region, possibly indicative of a supermassive black hole at its core. There does not appear to be any significant tidal disturbance or evidence of a recent major merger. The presence of a faint blue light in the disk may indicate some star formation.
