The galaxy presents a somewhat amorphous shape with an overall smooth appearance. The light distribution suggests a centrally concentrated morphology, possibly elliptical or lenticular. There is an indication of an extended halo or diffuse light surrounding the central region. A degree of asymmetry is observed, with a potential disturbance in the morphology, suggesting a possible interaction or ongoing merger event with another, smaller body. The color profile displays a gradient, transitioning from a redder core to slightly bluer outskirts, indicative of varying stellar populations and ages within the galaxy. Star formation appears to be present but at a relatively low rate.
