The galaxy presents as a somewhat smooth, though not perfectly elliptical, structure. There is evidence of a bulge. The color distribution suggests a variation in stellar populations or dust content across the galaxy. One side displays a more reddish hue, potentially indicating older stars, dust obscuration, or a higher concentration of cooler stars. The opposite side exhibits a bluer color, which may suggest regions of more active star formation and younger, hotter stars. The galaxy appears to be generally isolated, although some asymmetry in the outer regions could indicate past or ongoing gravitational interactions. No prominent spiral arms or strong bar structures are clearly visible. There are only slight disturbances in the outer area of the galaxy.
