The galaxy presents a largely smooth, centrally concentrated morphology. It appears elliptical or possibly a lenticular galaxy, displaying a high degree of radial symmetry. The core region exhibits a bright, yellowish hue, likely indicating a population of older, redder stars. Moving outward from the core, the galaxy gradually transitions to a slightly bluer tint, suggesting the presence of a younger stellar population, but the lack of defined spiral arms suggests the star formation rate is low. The isophotes of the galaxy appear generally regular and undisturbed, indicating no recent major merger events. There are no obvious signs of dust lanes or prominent star-forming regions within the galaxy's disk. The overall appearance is consistent with a fairly evolved galaxy with a stellar mass slightly above average, with a low specific star formation rate.
