The observed galaxy presents as a disk-dominated system, exhibiting a notable degree of smoothness in its overall structure. The central bulge is prominent, displaying a bright, concentrated luminosity. Proceeding outwards, the disk gradually fades, forming a somewhat diffuse and elongated morphology. The overall ellipticity suggests a significant inclination with respect to our line of sight. There are no readily apparent spiral arm structures or distinct star-forming regions visible in this imagery. The smooth texture and lack of prominent features points toward an older stellar population. No major merger events or tidal disturbances are obvious, although minor disturbances cannot be entirely ruled out. The galaxy shows a color gradient, the center tending to be a little whiter, and the outer disk tending to be a little redder. The galaxy's intermediate apparent roundness suggests it falls between a perfectly circular and elongated shape.
