The galaxy presents as a single, relatively bright object with a smooth, somewhat elliptical morphology. The primary body appears rounded, with a concentrated central bulge. The color gradient suggests an older stellar population dominating the central regions, transitioning toward slightly bluer, potentially younger stars in the outskirts. A faint tidal tail extends from the main body of the galaxy, possibly indicative of a past interaction or merger event. This tail exhibits a redder color, indicating a lower star formation rate or dust obscuration compared to the central region. The galaxy appears relatively isolated, with no obvious signs of ongoing major interactions.
