The galaxy presents as a generally smooth object with a moderate degree of ellipticity. A central bulge is apparent, exhibiting a yellowish hue, suggesting an older stellar population and/or a higher concentration of dust obscuring bluer wavelengths. The outer regions of the galaxy appear fainter and less defined, showing a hint of a disk-like structure extending outwards. There is a slight color gradient from the core to the outer regions, with the outer areas tending towards bluer shades. There may be some evidence of subtle disturbances or asymmetry in the disk, although a clear classification of spiral arms or other distinct features is not possible based on the available image resolution. The overall appearance indicates a galaxy that is neither perfectly elliptical nor a well-defined spiral, residing somewhere in between.
