The galaxy presents as a single, relatively smooth, centralized object, likely a spheroid or elliptical galaxy, with minimal signs of spiral arm structure or significant disk components visible in this imaging. Its light is somewhat evenly distributed, exhibiting a radial gradient.

There is a slight yellowish hue, which could indicate an older stellar population and relatively little ongoing star formation. The galaxy appears moderately compact, with a concentration of light towards the center, but also a faint extension of luminosity in its outer regions.

The overall shape of the galaxy appears somewhat elongated, though it may be closer to round. There does not appear to be evidence of any major ongoing merger events or significant tidal disturbances affecting the galaxy's structure. The object appears relatively isolated.
