The galaxy exhibits a smooth, elliptical morphology with a concentrated central bulge. The overall color is relatively uniform, trending towards redder hues which suggests an older stellar population with suppressed star formation. There is a noticeable absence of distinct spiral arms or prominent dust lanes. The galaxy appears undisturbed, showing no major signs of tidal interactions or recent mergers. Its shape is approximately in between round and elliptical. There is minimal evidence of ongoing star formation activity based on the color profile. The galaxy is likely a mature system with a considerable stellar mass.
