This galaxy presents as a disk galaxy, though the classification is somewhat uncertain. The primary disk component is oriented at a significant inclination relative to our line of sight, possibly approaching edge-on. There is a noticeable bulge at the galaxy's center, which appears yellowish, indicative of an older stellar population. Fainter blue regions are present within the disk, suggesting ongoing star formation. Irregularities and disturbances are seen within the disk which indicate a recent merger or tidal disturbance. A plume-like feature is visible extending away from the galaxy, potentially a tidal tail formed during an interaction. There is a second dimmer object underneath the galaxy which may be part of a merging system. 
