The galaxy presents as a relatively compact system. A significant portion of its light originates from a bright, centrally concentrated region, suggesting a prominent bulge or core. The overall form appears somewhat elliptical, though it's not perfectly symmetrical. There's a hint of an extended feature or arm extending from the main body of the galaxy, appearing as a slight disturbance or merging object. The system's color profile indicates active star formation, particularly within that extended feature. This suggests the presence of younger, bluer stellar populations alongside older, redder stars. The galaxy's overall light profile suggests it is a moderately massive system with ongoing star formation. The observed asymmetries further imply a dynamic history, possibly involving interactions with smaller galaxies.
