The galaxy presents a disk-like morphology when viewed from our perspective. Its angular size is relatively small. The galaxy's color profile suggests the presence of both older stellar populations and regions of recent or ongoing star formation. A central bulge is not clearly discernible. Faint spiral arm structures are present. Patches of bluer light are evident, indicating star-forming regions or populations of young, hot stars, with slightly redder regions possibly indicative of dust lanes or more evolved stellar populations. No strong evidence of a major merger is apparent. There may be slight disturbances in the disk. The galaxy's shape appears somewhat distorted, suggestive of a possible interaction or tidal effect. The overall impression is of a relatively normal, moderately inclined spiral galaxy, with some hints of past or current interactions influencing its structure.
