The galaxy presents a predominantly smooth morphology, exhibiting a slightly elongated, cigar-like shape. The central region appears brighter and more concentrated, suggesting a higher density of stars and possibly an older stellar population, indicated by the yellowish hue. The outer regions display a bluer tint, potentially indicative of ongoing or recent star formation. There is little evidence of distinct spiral arms or a well-defined disk structure, but a slight flattening is apparent. No major disturbances, mergers, or tidal features are readily discernible.
