The galaxy presents an elliptical morphology, exhibiting a smooth, luminous profile. The core region displays a concentrated brightness, gradually diminishing towards the outer edges. The galaxy possesses a yellowish hue, which is consistent with an older stellar population. The presence of a smaller, seemingly interacting galaxy is also detected nearby, exhibiting signs of distortion. This smaller galaxy has a bluer hue compared to the primary galaxy. The overall structure suggests a possible recent or ongoing galactic interaction, potentially a merger event.
