The galaxy appears to be a relatively smooth, elliptical system. The light distribution suggests a concentrated central bulge, with a gradual decrease in luminosity towards the outer regions. There is no evidence of prominent spiral arms or a distinct disk structure. The color gradient suggests a population of older stars, with a yellowish hue dominating the central region. There is faint blue emission in the outer regions, indicating some low level of on-going star formation activity. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger or tidal interactions. The overall morphology is consistent with an early-type galaxy at a moderate redshift.
