The galaxy presents as a concentrated, luminous object with a generally smooth morphology. It is characterized by a central bulge that exhibits a yellow-orange hue, indicative of an older stellar population with a dominance of redder giant stars. The overall shape appears to be somewhat elliptical but has some disturbances. There are two distinct bright lobes or cores apparent within a central, somewhat disorganized or disturbed region. There is a small companion galaxy appearing very nearby, and seems to be within the same structure as the main galaxy. This is suggestive of a possible interaction or ongoing merger event between the two galaxies. Overall, the system does not display prominent spiral arms or significant dust lanes that are easily discernible. This suggests that star formation within this galaxy is likely subdued, with a relatively low rate of new star formation.
