The galaxy presents as a significantly elongated, spindle-shaped morphology. It exhibits a generally smooth profile with no immediately discernible spiral arms or bar structures. A prominent central bulge appears bright and concentrated, emitting light primarily in the redder wavelengths, suggestive of an older stellar population. Fainter, bluer light extends along the major axis, tapering towards the extremities of the galaxy. This could be indicative of ongoing, albeit limited, star formation within the disk. No major merger events or tidal disturbances are immediately obvious; however, subtle asymmetries in the outer regions cannot be ruled out without further spectroscopic or higher-resolution imaging. The galaxy’s overall color is intermediate between a pure elliptical and a spiral galaxy, potentially representing an intermediate stage in galaxy evolution.
