This galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a bright, yellowish-white hue, indicative of an older stellar population and/or dust attenuation. The galaxy's overall color appears slightly redder than that of other galaxies, possibly due to its redshift, or the dominance of older, redder stars. There appears to be some distortion in the shape. While the overall light distribution is relatively uniform, there are subtle hints of a faint, extended halo surrounding the central region. There's some evidence of potential interaction in the form of slight irregularities along the edges and minor light asymmetries.
