This galaxy appears to be a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy. The light distribution is fairly symmetrical, with a gradual decline in surface brightness from the core outwards. There is a hint of a possible disk structure or some feature component extending from the central region, but it is not clearly defined. The galaxy's color suggests an older stellar population, being more reddish in appearance. There is no evidence of strong spiral arms or active star formation regions. The galaxy appears relatively isolated with only minor disturbances.
