The galaxy presents as a relatively smooth and concentrated object, with evidence of a prominent bulge. The light distribution suggests a centrally dominant spheroid component. The morphology appears largely undisturbed, although there might be minor asymmetries or faint extensions detectable. The color profile indicates an older stellar population dominating the central regions, exhibiting a yellowish hue. There is also evidence of bluer light concentrations offset from the center, possibly indicative of ongoing star formation. Overall, this galaxy appears to be a relatively massive system, likely with ongoing though potentially subdued star formation activity.
