The galaxy presents a largely smooth morphology, displaying a central bulge that dominates the overall luminosity. There is little evidence of a prominent disk structure. The galaxy appears slightly elongated, deviating marginally from a perfect circular shape. Possible minor disturbances exist within the structure. The object exhibits a colour gradient, with a subtly redder hue concentrated towards the central region, which implies the presence of an older stellar population and suggests star formation is not the dominant process.
