The object appears to be a spiral galaxy, observed at a slight inclination relative to our line of sight. The central bulge is prominent and appears yellowish, suggestive of an older stellar population. Faint, loosely wound spiral arms extend outward from the bulge. These arms appear slightly bluer in color than the central bulge, indicating the presence of younger, hotter stars. A weak bar feature may be present across the central region. There is no significant morphological disturbance, though the galaxy appears to be undergoing a minor interaction.
