The galaxy presents a roughly circular morphology, displaying a centrally concentrated luminosity profile. The core region exhibits a bright, cyan hue suggestive of active star formation or a strong emission line signature. Surrounding this central region, a faint, diffuse halo extends outwards. Within this halo, subtle color variations are observable, with a gradient from cyan towards greenish-yellow in some areas, hinting at variations in stellar populations or dust content. Redder regions are also visible, but they are less concentrated and may suggest the presence of dust lanes, older stellar populations, or possible tidal disruptions. Based on the irregular and broken outer edges and faint tidal tails, the galaxy appears to be undergoing minor morphological disturbance, perhaps due to a recent or ongoing interaction or merger. The smoothness of the central core implies that it is unlikely that it is undergoing a major interaction.
