The galaxy appears as a moderately luminous object with a generally elliptical morphology. The core region exhibits a reddish hue, possibly indicative of an older stellar population and a lack of ongoing star formation in the central region. Faint blue emissions at the edges suggests more recent or ongoing star formation. Overall, it seems to be a very massive galaxy, but exhibits a low star formation rate. Some kind of potential gravitational interaction with nearby objects might explain some disturbances visible in the structure.
