The galaxy appears to be a spiral galaxy, viewed at a slight angle. It presents a generally smooth appearance, with a notable central bulge. A faint disk is discernible, exhibiting arm-like structures which suggests ongoing, though perhaps subdued, star formation. The color profile indicates the presence of both older stellar populations as well as areas of younger, bluer stars, especially within the hinted spiral arms. There is a possible interaction or merging event underway, with some visible asymmetry within the galaxy's structure, possibly induced by tidal forces. The galaxy's roundness suggests it's likely at a relatively early stage of disturbance, or experiencing a minor gravitational interaction. Overall, the galaxy seems to be a mid-mass system, likely undergoing a period of transition or evolution.
