The galaxy appears to be an early-type spiral, likely a lenticular or Sa type, with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. A faint disk is observed, but the spiral arms are not clearly defined.

There appears to be a potential minor merging event or tidal disturbance visible. A small, bluish object is observed in close proximity to the main galaxy, suggesting an interaction with the central galaxy. It seems to be relatively high in star formation. There may be ongoing tidal disruptions. This could indicate past or present minor merger activity. Overall, the galaxy presents some evidence of a potential interaction or disturbance.
