The galaxy presents a smooth, elliptical morphology with no obvious spiral arm structure. The light distribution is centrally concentrated, with a bright, yellowish core that gradually fades into the outer regions. The galaxy exhibits a moderate ellipticity, appearing more elongated than perfectly spherical. There may be slight irregularities in the outer regions, but these appear to be very minor. The overall color of the galaxy appears to be relatively red, suggesting an older stellar population. There is no clear evidence of ongoing major star formation, although there may be some. The galaxy seems to be relatively isolated, with no obvious signs of a major merger event in its recent history.
