The galaxy presents a largely smooth morphology. The light distribution is dominated by a central bulge, which appears roughly spherical and emits strongly in the redder bands. There is a subtle color gradient, the core exhibiting a yellower hue, transitioning to a redder tint towards the outer regions. This may indicate a decrease in metallicity or age of stellar populations with increasing radius. There is some evidence of faint disk-like features, but the dominant morphology is spheroidal. It seems to be a relatively massive system, and is likely an elliptical galaxy. There might be minor disturbances that warrant further investigation with higher resolution imaging.
