The galaxy presents as a roughly elliptical structure, appearing generally smooth with a concentrated central bulge. The core exhibits a yellowish-white hue, possibly indicative of an older stellar population. The outer regions of the galaxy are less defined, fading into a greenish halo. There is some evidence of mild tidal disturbances or asymmetries, potentially from past minor interactions, but there is no clear sign of an ongoing major merger event. Overall, the galaxy appears as a massive system, likely undergoing moderate levels of star formation.
