The galaxy presents as a somewhat diffuse, disk-like system, exhibiting a centrally concentrated brightness profile. The overall shape appears moderately elliptical with the main body of the galaxy spanning approximately 6 arcseconds. The light distribution is relatively smooth, with a slightly elongated, rather than spherical shape.

There is a discernible difference in color between the central region and the outer regions. The core appears to be a more uniform white color, while the outer regions exhibit a bluer hue. This might suggest differing stellar populations, with older, redder stars concentrated in the core and younger, bluer stars more prevalent in the disk. 

There is some indication of disturbance, possibly interaction with another galaxy. A portion of the galaxy appears as a minor disturbance within its structure. The light distribution is not perfectly smooth, and there may be some signs of tidal features or asymmetries, but the image quality makes further classification uncertain.
