The galaxy presents as a somewhat elongated, elliptical form. There is a noticeable central bulge, characterized by a yellowish hue, suggesting an older stellar population. The outer regions exhibit a fainter, bluer tint, potentially indicating areas of more recent or ongoing star formation, with younger, hotter stars. The galaxy appears relatively smooth, with no obvious spiral arm structure visible in this image, though there may be a slight asymmetry to the shape of the outer regions. The axial ratio indicates a moderate ellipticity, suggesting it is not viewed face-on, but rather at a slight angle to our line of sight. Overall, this galaxy appears to be a relatively massive system undergoing some degree of star formation.
