The galaxy presents a generally smooth morphology, although some internal structure is faintly discernible. The light distribution appears elongated, with a high degree of ellipticity. The central region exhibits a brighter, more concentrated luminosity profile, suggesting a possible bulge. The color gradient transitions from a yellowish-white core to a slightly bluer hue in the outer regions, which could indicate the presence of younger stellar populations further from the center. There is no strong evidence of a recent major merger or significant tidal disturbances, but there is some very slight visible disturbance. It displays an estimated mass typical of a large galaxy, but a low star formation rate for a galaxy of this size.
