The galaxy presents a largely elliptical morphology, exhibiting a smooth and concentrated light profile. The color is noticeably redder compared to typical spiral galaxies, likely indicative of an older stellar population and reduced ongoing star formation. There's a slight asymmetry in the light distribution, hinting at potential minor disturbances or interactions, but the overall structure appears relatively undisturbed. The galaxy's half-light radius suggests it is a moderately sized galaxy. The absence of prominent spiral arms or a well-defined disk further supports the classification as an elliptical galaxy with an older stellar population and lower rates of star formation.