The galaxy appears as a centrally concentrated object with a relatively smooth, elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the center, the color shifts towards a bluer tone, hinting at the presence of younger stars or ongoing star formation in the outer regions. There is little evidence of distinct spiral arms or prominent dust lanes. The galaxy does not appear to be undergoing any major merging events, though there is a slight distortion to its shape that may point to a minor interaction. Overall, the object presents as a moderately massive system with a mix of stellar populations, predominantly an elliptical form with a hint of disky features.
