The galaxy presents a generally smooth morphology with a prominent bulge. It exhibits a flattened disk structure, though details are somewhat obscured by the image resolution. The galaxy's color profile suggests a population of older stars, with a noticeable concentration of yellow and orange hues. The overall shape is closer to elliptical, although not perfectly spherical, presenting as an in-between form. Indications suggest a minimal disturbance, without strong evidence of ongoing major merging events.
