The galaxy presents as a diffuse, somewhat irregular structure, possibly indicative of a galaxy undergoing a merger or showing signs of significant disturbance. It has a general bluish hue, most notably visible on the upper left region, which suggests the presence of younger, hotter stars and ongoing star formation. The overall luminosity appears to be relatively faint, and the galaxy is not particularly well-defined, with indistinct edges and a mottled appearance. There is a hint of reddish color within the central regions and on the bottom of the galaxy which is a possible indication of older stellar populations. No clear spiral arms or a distinct central bulge are readily apparent.
