The galaxy presents as a relatively smooth, elliptical form. Its shape appears elongated, with a clear major axis. A concentration of light is observed toward the center of the galaxy, suggesting a prominent galactic nucleus. There's a noticeable color gradient from the center outwards, transitioning from a reddish hue in the core to a blue-green tint in the outer regions. The light distribution suggests that the galaxy is likely an early-type galaxy, specifically elliptical or lenticular. The overall smooth appearance indicates a lack of prominent spiral arms or significant dust lanes, supporting the hypothesis of an older stellar population with relatively low ongoing star formation. There may be a very small degree of interaction with another galaxy, but there is no obvious sign of such interaction.
