The galaxy presents a somewhat smooth appearance overall. Its morphology is elongated, with a shape between round and cigar-shaped, suggesting it may be a disk galaxy viewed edge-on. There is a subtle, but noticeable central bulge. The galaxy doesn't show any clear signs of major disturbance or merging activity, although some minor disturbance cannot be entirely ruled out. Based on the colors, the galaxy is likely a relatively low-mass galaxy with a low star-formation rate. The color implies a generally older stellar population, though there may be a small component of younger, bluer stars.
