The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile transitions from a redder hue at the core to a slightly bluer tint in the outer regions, suggesting a potential gradient in stellar populations with older, redder stars concentrated centrally and possibly younger, bluer stars in the outer regions. While the galaxy's overall form is mostly smooth, there is a slight hint of asymmetry or a minor disturbance in its shape, possibly indicative of past or ongoing interactions with a companion. No strong spiral arm structures or prominent dust lanes are discernible. The light distribution appears generally centrally concentrated. Overall, it seems to be a relatively massive galaxy with an intermediate redshift, consistent with a mature stellar population and a moderate star formation rate.
