The galaxy presents as a somewhat elongated structure. The central bulge appears bright and has a yellowish hue, which may indicate an older stellar population residing in this region. Surrounding the bulge, a faint disk structure is visible with bluish tones, suggestive of younger, hotter stars and ongoing star formation. The disk is not well-defined, lending a relatively smooth appearance to the galaxy as a whole. There appears to be a slight asymmetry in the galaxy's morphology, with one side of the disk possibly being more extended or disrupted than the other, though it is not clear whether this is due to an interaction or internal processes. There is no strong evidence of significant spiral arm structure or a prominent bar. The overall color gradient implies a decrease in stellar age from the center to the outer regions.