The galaxy presents as a centrally concentrated object, with a smooth, diffuse light distribution. It appears largely elliptical in shape, tending toward a somewhat rounded morphology rather than an elongated, cigar-like structure. There is a hint of a faint, extended halo surrounding the central region. While the galaxy appears mostly undisturbed, there is a possible minor irregularity or a slight asymmetry, indicating a potential recent interaction or internal disturbance. The galaxy exhibits a color gradient with a central, brighter region appearing nearly white, gradually transitioning to a slightly redder hue towards the outer edges, suggesting a centrally concentrated population of stars.
