This galaxy appears to be a relatively small, elongated system. Its shape is predominantly cigar-shaped, lacking prominent spiral arms or a well-defined bulge. The color distribution suggests a central region that is bluer than its outer edges, indicating potential ongoing star formation in its core. However, the overall lack of distinct features points towards a significant fraction of older stellar populations. There is little evidence of major disturbances or merging activity, suggesting a relatively stable, isolated system.
