The galaxy presents as a relatively smooth, elliptical or lenticular structure. The central bulge is bright, exhibiting a yellowish hue, suggesting a population of older stars. A subtle disk-like component appears to be present, with a slight elongation along a particular axis. This disk shows evidence of bluer tones, possibly indicating regions of recent, though limited, star formation. The outer regions of the galaxy fade gradually, appearing less concentrated than the core. There is no clear indication of any major mergers or significant tidal disturbances; any interactions appear to be relatively minor. The galaxy is generally well-defined, exhibiting a moderate size relative to other galaxies in the image set.
