The galaxy presents as a relatively compact object, exhibiting a somewhat elliptical morphology. There appears to be a central concentration of light, indicating a possible bulge or core region. The overall color is skewed toward the redder end of the spectrum, suggesting a population of older stars. The galaxy shows possible signs of interaction, indicated by a double lobed morphology. There is no obvious spiral structure visible. It appears largely smooth, with possible signs of an ongoing or recent merger event.
