The galaxy presents as a relatively smooth, elliptical structure with an apparent moderate ellipticity. The light distribution suggests a centrally concentrated bulge, with a gradual falloff in brightness towards the outer regions. A subtle disk-like feature appears embedded within, presenting a potential for ongoing star formation, as indicated by its slightly bluer color and regions of clumpy star formation. Overall, the galaxy appears to be an intermediate-mass system, perhaps undergoing some form of minor interaction or disturbance, influencing its shape and star formation rate. This galaxy has a redshift of about 0.065.