The galaxy presents as a relatively smooth, centrally concentrated object with a yellowish hue. There is minimal evidence of spiral arm structure or prominent dust lanes. The overall shape appears approximately round, lacking significant elongation or asymmetry. Color gradients suggest a possible radial variation in stellar populations, with a potentially older, redder population dominating the core. The galaxy exhibits a degree of faint, diffuse light extending beyond the central region, indicating a halo component. Given the smooth appearance, it is likely an elliptical galaxy or a lenticular galaxy. There is no indication of a major merger event or significant tidal disturbances.
