The galaxy presents as a slightly inclined disk galaxy. The central bulge appears relatively prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. A fainter, bluer disk surrounds the bulge, indicating the presence of younger stars and potential ongoing star formation. There is evidence of some irregularities or disturbances within the disk structure; while a distinct spiral arm structure is not apparent in this image, a patchy distribution of light suggests some non-uniformity in the distribution of stellar material. Overall, the galaxy appears to be relatively isolated.
