The galaxy presents a generally smooth appearance, with a notable elliptical morphology. The light distribution suggests a dominant spheroidal component. The galaxy exhibits a color gradient, transitioning from a more yellow-red hue in its central regions to a slightly bluer shade towards its outer edges. No prominent spiral arms or distinct dust lanes are visible. The galaxy's shape is elongated, appearing somewhat cigar-shaped. There is no obvious indication of a major ongoing merger event, though a minor asymmetry or disturbance cannot be entirely ruled out. Star formation rate appears to be relatively low.
