The galaxy presents as a moderately luminous object with a relatively smooth morphology. It appears somewhat elliptical in shape, exhibiting a gradual fading of intensity from the core outwards. A slight hint of disk-like structure may be present, though the overall form is dominated by a bulge or spheroidal component. There are no obvious signs of strong spiral arms or bar structures. The color profile suggests a population dominated by older stars, as indicated by the redder hues. There is no clear indication of any major ongoing merger activity, though a minor disturbance cannot be entirely ruled out.
