The galaxy presents a somewhat diffuse appearance, exhibiting a central concentration of light that suggests a bulge. The light from the bulge is yellowish, indicating an older stellar population. Extending outward from the central region are fainter, less defined structures. There are no clear spiral arms, but there is some evidence of disk-like features. The overall color of the outer regions is bluer, suggesting the presence of younger, hotter stars. The image hints at some disturbances in the galaxy's structure, with a slight asymmetry. It is uncertain if these are due to tidal interactions, or if they are simply internal to the galaxy. There is a lack of strong star-forming regions visible in this image. The galaxy appears to be relatively isolated within its field. The galaxy's size seems moderate.
