The galaxy presents as a fairly smooth object with an elongated, cigar-like morphology. A central bulge region is discernible, appearing more concentrated and exhibiting a yellowish hue. This suggests a population of older stars in the core. The overall color gradient indicates a shift towards redder wavelengths from the inner regions to the outer edges, potentially indicating a decreasing density of younger, bluer stars towards the periphery. No distinct spiral arms or prominent dust lanes are readily visible. The lack of significant morphological disturbances and the smooth appearance suggest it is likely an early-type galaxy, either an elliptical or a lenticular galaxy. There is no apparent interaction or merging activity evident from this single image.