The galaxy presents as a centrally concentrated, smooth object with a yellowish hue. It appears largely spheroidal, displaying little evidence of spiral arms or other distinct features. The light distribution suggests a relatively old stellar population dominating the galaxy's overall luminosity. There is a subtle extension of light around the central bulge, possibly indicating a faint disk or halo component, but it is not well-defined. There is no obvious tidal distortion or signs of a major merger, although the possibility of a minor interaction cannot be entirely ruled out given the image resolution.
