The galaxy appears to be a relatively compact, smooth object. Its light is centrally concentrated, with a gradual decrease in intensity towards the outer edges. There is no strong evidence of spiral arms or a distinct disk structure; rather, the galaxy exhibits a generally elliptical appearance. The overall color seems to be somewhat redder than average, suggesting an older stellar population. No significant morphological disturbances or tidal features are readily apparent. The galaxy appears isolated, showing no obvious interactions with nearby galaxies. It is fairly bright for its size.