The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a fairly elliptical shape, appearing mostly round with a slight elongation. There is no obvious spiral arm structure or bar. The light distribution indicates a prominent bulge, which dominates the galaxy's overall appearance. The galaxy exhibits a color gradient, with a reddish hue towards the center, transitioning to bluer tones in the outer regions, suggesting a potential difference in stellar populations or dust distribution. There is no strong evidence of significant tidal disturbances or ongoing major mergers based on the visible structure. Faint, diffuse light extends outwards from the main body of the galaxy, forming a halo.
