The galaxy presents as a relatively compact object. It exhibits a subtle yet discernible red hue, suggesting a population of older stars and/or significant dust obscuration. There appears to be a central concentration of light, possibly indicative of a bulge or core region. The overall morphology leans toward a smooth appearance, with little evidence of spiral arms or other distinct features. The light is relatively faint. There is a very slight, but clear extension of light to one side of the object. Given the relatively uniform color distribution, internal star formation appears minimal. There is no visual evidence of a recent or ongoing major merger. Faint disturbances may be present.
