The galaxy presents as a moderately luminous object at a redshift of approximately 0.15. It appears as a centrally concentrated mass, with a shape that appears to be in-between elliptical and disk. The galaxy displays a mostly smooth light distribution, with some small indications of faint substructure. The central bulge dominates the overall light profile. There is some evidence of slight disturbance, but it is not undergoing a major merger. In the optical bands, the galaxy exhibits a color gradient, appearing bluer towards the outer regions. This could potentially indicate regions of ongoing star formation, albeit at a relatively low rate.
