The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. The core region appears significantly brighter and takes on a yellow hue, suggesting a population of older stars dominating this area. Moving outward from the center, the light decreases gradually. Faint reddish tones can be discerned at the edges of the galaxy, which may indicate older stellar populations or dust absorption. It does not appear to be undergoing a major merger event, and displays no strong disturbances in its overall structure. The galaxy is elongated with an aspect ratio greater than one. Based on the galaxy's color and structure, it is likely a galaxy with very little on-going star formation.
