The galaxy presents an elliptical morphology, elongated in shape with a relatively smooth overall appearance. There is a noticeable concentration of light toward the central region, forming a bright core. The color profile indicates a generally older stellar population, shifting from yellow in the center to slightly bluer hues in the outer regions. The galaxy does not display any prominent spiral arms or significant dust lanes. It appears to be relatively isolated, without obvious signs of major interaction or disturbance from neighboring galaxies. The elongation suggests a slight flattening and potentially some rotational support.
