The galaxy presents as a moderately sized, relatively smooth object with a concentrated central bulge. It exhibits a subtle, elongated morphology, neither perfectly spherical nor highly flattened. The color profile indicates a population of older stars, with a dominant reddish-yellow hue, suggesting lower recent star formation rates. There is a slight indication of possible minor disturbances or interactions, evidenced by faint asymmetry in the outer regions of the galaxy. However, a definitive merger classification is uncertain based on this imagery alone. The overall structure suggests an early-type galaxy, potentially an elliptical or lenticular, with limited ongoing star formation.
