The galaxy presents a roughly elliptical morphology. The light distribution suggests a central bulge region that appears bright and relatively smooth, surrounded by a fainter, more extended disk. There is evidence of some structural features within the disk, potentially indicating spiral arm segments or irregular star-forming regions. 

The color gradient across the galaxy suggests a possible age or metallicity difference between the central bulge and outer disk. The bulge appears bluer compared to the disk, which shows a hint of redder tones. There appears to be a slightly irregular structure, potentially indicating a minor interaction or ongoing merger event. The overall appearance hints at a galaxy that is neither a purely elliptical nor a well-defined spiral, but possibly an intermediate type or one undergoing some form of morphological transformation.
