The galaxy appears to be a relatively compact object. It exhibits a predominantly smooth morphology, lacking any obvious spiral arms or bar structures. There is evidence of a slight central concentration of light, hinting at a possible core or bulge region. The overall color of the galaxy is a somewhat yellowish to slightly reddish hue, implying a population of older stars, but the core seems to have a bluer tint. There are possible disturbances to the galaxy indicating there may be a merger occurring.
