The galaxy appears as a slightly elongated, diffuse object. It exhibits a predominantly smooth morphology with a central concentration of light, suggesting a possible bulge. There is evidence of a fainter, disk-like structure surrounding the core. The color profile indicates a bluish hue, particularly within the disk, suggesting the presence of younger, hotter stars and ongoing star formation. The galaxy does not show obvious signs of strong tidal interactions or major mergers, though there may be some minor disturbances apparent in the outer regions of the disk. The overall structure suggests a galaxy somewhere between a pure elliptical and a fully formed spiral, potentially an intermediate disk galaxy.
