The galaxy presents as a generally smooth object with a noticeable elongation. Its color profile suggests a composition dominated by older stellar populations, as evidenced by the reddish hues observed, particularly at the galactic bulge. There is a suggestion of a faint disk component oriented along the major axis, though distinct spiral arms are not apparent. The color gradients indicate a slight central concentration of bluer, possibly younger stars, toward the core. The overall morphology is consistent with an elliptical or lenticular galaxy type, displaying a relative lack of ongoing star formation. There are no obvious signs of tidal disturbances or interactions with other galaxies in its immediate vicinity.
