The galaxy presents a relatively smooth and centrally concentrated morphology, appearing somewhat elliptical in shape. The dominant color is a yellowish-orange hue, suggesting an older stellar population, particularly in the central bulge region. There is little evidence of distinct spiral arm structure or significant dust lanes, though a slight asymmetry in the outer regions could suggest the presence of a faint, disturbed disk. The galaxy does not appear to be undergoing a major merger, although a minor interaction or disturbance cannot be ruled out based on the faint asymmetry observed. Overall, the galaxy appears to be a moderately massive system with a relatively low star formation rate.
