The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated morphology. The light profile is dominated by a bright, relatively spherical core that fades gradually outward. The galaxy's overall shape is slightly elongated, tending towards a cigar-like appearance rather than being perfectly circular. There's a subtle color gradient present, with the central region showing a yellowish hue, suggesting a population of older stars, while the outer regions appear slightly bluer, which may indicate the presence of younger stars or a small amount of ongoing star formation. There are no distinct spiral arms or prominent dust lanes visible. The galaxy does not appear to be undergoing a major merger, though there are subtle signs of minor disturbance or interaction that have changed the shape.
