The galaxy presents as an elliptical system, showing a smooth, centrally concentrated luminosity profile. The core region exhibits a bright, golden-hued glow, which gradually fades towards the outer edges. The galaxy has an elongated shape, appearing close to round but slightly oval. The overall color suggests an older stellar population with minimal dust obscuration, likely indicating a low current star formation rate. No distinct spiral arm structure or prominent dust lanes are discernible. Minor disturbances seem to be ruled out due to the smoothness of the profile. The light distribution appears consistent with a Sersic profile, potentially suggesting a classification as an elliptical galaxy. 
