The galaxy presents a generally smooth appearance with a somewhat elongated, cigar-shaped morphology. It exhibits a color gradient, appearing bluer at one end and redder at the other. There is a suggestion of some disk structure, but no prominent spiral arms are visible. There may be a slight disturbance in the galaxy's structure, potentially indicating a minor interaction or internal activity. Overall, the galaxy doesn't appear to be undergoing a major merging event, but some level of gravitational interaction or internal dynamic process cannot be ruled out.
