The galaxy presents as an object with a notable degree of smoothness in its overall structure, suggesting a relatively evolved morphology. It appears to be dominated by a large spheroidal component. There is a slight degree of elongation, though the galaxy is generally roundish in appearance. Indications of disturbances and interactions are present. The redder hue in the central region may signify an older stellar population. While there is no definitive evidence of spiral arm structure, subtle bluer areas might indicate some star formation activity occurring. A secondary object appears to be interacting with the galaxy or a close companion.
