The galaxy appears as a relatively smooth, elliptical-like structure. There is a distinct central bulge, exhibiting a yellowish-gold hue, suggesting a population of older, redder stars. Moving outwards from the center, the light becomes slightly bluer, indicating some presence of younger, hotter stars, although their contribution appears limited. There are no obvious spiral arms or bar structures visible. The overall form is generally round with a slight cigar shape to it, fading into the background sky without any distinct edges. There are no indications of ongoing major mergers or significant tidal disturbances.
