The galaxy presents a generally smooth morphology, with a concentrated central bulge. The overall shape appears largely spheroidal, showing little evidence of a disk-like structure. There are no obvious signs of spiral arms or significant dust lanes. The galaxy's color gradient suggests a population of older stars, with the central region exhibiting a yellowish hue. This is suggestive of a more passive or quiescent galaxy, potentially indicating limited ongoing star formation. The absence of prominent features supports the classification of this galaxy as likely elliptical, with no major interactions or disturbances readily apparent.
