This galaxy presents as an elliptical-type morphology, though subtle features suggest a possible disk component. The galaxy exhibits a moderately smooth appearance overall, with a centrally concentrated luminosity profile. There is some evidence of minor disturbance in the form of slight asymmetries in the outer regions, hinting at a potential past or ongoing interaction. Color gradients within the galaxy appear subtle, with a trend towards redder hues in the core region. Overall, the galaxy is relatively compact in size with an appreciable luminosity, possibly indicating a high stellar mass density.
