The galaxy presents as a diffuse, roughly elliptical object. Its light distribution is dominated by a smooth, centralized bulge, indicating a potentially older stellar population. There is only a faint hint of a disk component. The color appears to be relatively uniform across the galaxy, exhibiting a yellowish-orange hue, characteristic of evolved stars with suppressed recent star formation activity. There is no obvious evidence of strong spiral arm structure or active star-forming regions. The overall morphology suggests a system that is either an early-type spiral or a lenticular galaxy approaching the red sequence. The galaxy does not display any obvious signs of recent major merger events, though minor tidal disturbances or interactions cannot be entirely ruled out based on the available image.
