This galaxy appears to be a relatively smooth, centrally concentrated system. Its morphology suggests a likely elliptical galaxy, exhibiting a diffuse, somewhat amorphous structure. The central region displays a brighter, more condensed core, surrounded by a fainter, extended halo. There is very little evidence of spiral arms or significant disk features. The object exhibits a slight ellipticity but generally appears rounded. Overall, the galaxy seems to be relatively undisturbed, with only subtle indications of any past or ongoing interactions. The color distribution appears mostly uniform. The galaxy displays an absolute magnitude that suggests this is a galaxy of average size. The star formation rate is also relatively low. The image indicates that the galaxy's stellar population is composed primarily of older stars.
