The galaxy presents a somewhat blurred and distorted appearance, potentially indicating an ongoing or recent interaction with another galaxy. The main body exhibits a diffuse, elliptical morphology, with a smooth profile. The light distribution appears centrally concentrated, gradually fading towards the edges. There are noticeable asymmetries in the outer regions. A faint, extended tidal tail-like structure is observed emanating from one side, indicative of gravitational disruption. A secondary, less defined component or clump of material is positioned nearby, possibly a companion galaxy in the process of merging or a region of enhanced star formation triggered by the interaction. The color profile suggests a mixture of stellar populations, with a generally yellowish hue in the core, suggesting older stars, and hints of bluer regions in the outskirts, potentially indicating areas of more recent star formation. Overall, the galaxy's morphology suggests an actively evolving system likely undergoing significant gravitational interactions.
