The galaxy presents as a somewhat elongated, cigar-shaped structure. The central region exhibits a higher concentration of light, appearing more luminous and yellow-orange in color, suggestive of an older stellar population. Moving outwards from the core, the light gradually diminishes and transitions to a slightly bluer hue, potentially indicating the presence of younger, hotter stars or ongoing star formation within the galaxy's outer regions. There is some possible distortion visible in the disk.
