The galaxy appears as a relatively compact object, exhibiting a generally smooth morphology. There is a slight elongation, but overall it does not deviate significantly from a circular shape. The light distribution is concentrated towards the center, with a gradual decrease in brightness outwards. There is no obvious spiral structure or pronounced disk component visible. There may be some faint features suggesting minor disturbances, but these are not clearly defined and could be the result of image limitations. The color profile indicates the presence of a slightly older stellar population, as evidenced by the stronger intensity in redder bands compared to bluer bands.
