The galaxy presents as a slightly elongated, diffuse object with an overall bluish tint, suggesting active star formation regions. There appears to be some degree of disturbance or irregularity in its structure, possibly indicative of a minor gravitational interaction or internal dynamic processes. The main body of the galaxy displays a fairly smooth light distribution, though some clumping or knot-like features are discernible, concentrated towards the central area. Considering it is a relatively close galaxy, it is also a low-mass galaxy, and presents evidence of being a star-forming object.
