The galaxy presents a generally smooth morphology, appearing largely featureless in this image. It exhibits an elliptical shape, elongated but not excessively cigar-shaped. The light distribution indicates a concentrated central bulge. There is little evidence of spiral arms or a distinct disk structure. The color profile suggests a population of older stars, exhibiting redder hues, with a possible small area with younger stars. Indications of minor disturbances or interactions with other galaxies cannot be completely ruled out.
