The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. It exhibits a subtle elongation, suggesting a deviation from a perfectly circular shape, though the isophotes appear relatively regular. The luminosity profile rises steeply towards the center, culminating in a bright, well-defined nucleus. The overall color is moderately red, indicating a population of older stars and/or significant dust content. There is no discernible evidence of spiral arms or prominent star-forming regions. The galaxy appears to be an isolated system, with no apparent tidal features or nearby companions disrupting its morphology.
