The galaxy presents as a relatively compact object with an apparent smooth morphology. The overall shape is elongated, approaching a cigar-like form. There is evidence of internal structure, though details are indistinct. A subtle color gradient is observable, transitioning from a slightly bluer hue at the edges to a yellower central region. This color variation potentially indicates variations in stellar populations, with younger, bluer stars residing in the outer regions and older, redder stars concentrated towards the galactic center. No prominent spiral arms or dust lanes are discernible within the image. The object does not appear to be undergoing a major merger, though there might be some minor gravitational interaction occurring. Its mass is estimated to be large, and the star formation activity is low.
