The galaxy presents an overall elliptical morphology with a smooth light distribution, suggestive of an early-type galaxy. The central bulge is prominent, exhibiting a high concentration of light, with a yellowish hue indicating an older stellar population. There appears to be a slight elongation of the galaxy, but the lack of distinct spiral arms or clear disk structures further supports its classification as elliptical. There is no evidence of significant dust lanes or active star formation regions, consistent with a galaxy that has largely exhausted its gas supply. The galaxy appears relatively undisturbed, without any obvious signs of ongoing mergers or tidal interactions. The overall color suggests that the stellar population is dominated by older, redder stars.
