The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a generally round morphology, lacking any obvious spiral arm structures or significant disk features. There is little indication of any ongoing major mergers or tidal disturbances. The galaxy's color is relatively uniform, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Star formation activity is likely low or suppressed, as indicated by the lack of blue light which would be indicative of younger, hotter stars. The galaxy appears to be in a relatively quiescent state.
