The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The color appears to be primarily yellow-orange, suggesting a population of older stars and a low rate of ongoing star formation. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a high degree of roundness. There are no obvious signs of major tidal disturbances or ongoing mergers, suggesting the galaxy is relatively isolated and dynamically relaxed. Overall, the galaxy appears to be a quiescent elliptical galaxy dominated by an older stellar population.
