The galaxy appears as a relatively smooth, centrally concentrated object. The light distribution is dominated by a yellowish core, suggesting an older stellar population. There is a slight hint of extended, fainter material surrounding the core, exhibiting a redder hue. The overall shape is somewhat elliptical, though not highly elongated, with a notable absence of distinct spiral arms or irregular features. There is no visual evidence of ongoing mergers or tidal disturbances. The structure appears largely undisturbed, consistent with a galaxy that has undergone significant morphological quenching. Star formation is likely suppressed.
