The galaxy presents as a relatively smooth, elliptical morphology, exhibiting a concentrated central bulge. There appears to be little or no discernible spiral arm structure or significant dust lane features within the disk. The overall color is shifted towards the red end of the spectrum. The light distribution suggests that the galaxy is dominated by an older stellar population. There is no indication of strong ongoing star formation activity based on the observed color and lack of blue light. The galaxy seems to have a generally uniform and undisturbed structure, with no visual signs of recent mergers or major tidal interactions. The overall shape tends towards being round, although some ellipticity is still present.
