The galaxy presents as a somewhat elliptical structure, its major axis oriented approximately northeast to southwest. The central region exhibits a pronounced bulge with a concentrated, bright core, appearing yellowish, potentially indicating an older stellar population or significant dust obscuration. This core smoothly transitions to a less luminous, more diffuse halo. Traces of bluer light is visible near the edges of the galaxy, which may indicate regions of more recent star formation. The galaxy appears relatively smooth, lacking prominent spiral arms. A slight asymmetry in the outer regions hints at possible gravitational interactions or recent accretion events.
