The observed galaxy presents as an elongated, elliptical-like structure. The core region exhibits a high degree of luminosity, transitioning to a less intense glow towards the outer edges. There are some disturbances in the outer edges. The color profile is redshifted; the core displays a yellowish-orange hue that gradually fades into a redder tone in the surrounding regions. The galaxy doesn't appear to be undergoing any major merging activity, although there are slight disturbances that may be indicative of a minor interaction or internal process. Overall, the galaxy's morphology suggests a system dominated by older stellar populations with a modest star formation rate.
