The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated luminosity profile. The galaxy is roughly circular in shape, with no discernible spiral arm structures or bar features visible. It presents a relatively homogeneous color profile, showing a slight gradient from a bright, almost white core region fading to a blueish hue in its outer regions. There is no strong evidence of ongoing major merger events or tidal disturbances. It could possibly be a recently merged spiral galaxy that is relaxing into a more spherical form. Star formation rates are inferred to be low. The estimated size suggests a relatively compact structure.
