The galaxy appears as a relatively smooth, elliptical-shaped object. It exhibits a concentrated central bulge, characterized by a yellowish hue, suggesting an older stellar population. Moving outwards from the core, the galaxy gradually fades in brightness, transitioning to a slightly bluer color, possibly indicating the presence of younger stars in the outer regions, although star formation activity appears subdued overall. The galaxy's overall structure is largely undisturbed, lacking any prominent spiral arms or signs of ongoing major mergers. There might be some minor disturbances in the outer regions, but these are subtle. The object's elongation is moderate, falling between a perfectly circular and a cigar-like shape.
