The galaxy presents as a spiral type, characterized by a distinct disk-like structure. The central region exhibits a concentration of light, suggesting the presence of a bulge. Two prominent spiral arms emanate from this central bulge. These arms show a relatively well-defined structure, following a moderately wound pattern. There is no evidence of any major ongoing merger events or significant tidal disturbances, with the galaxy exhibiting a relatively unperturbed morphology. The disk is viewed at a slight angle relative to edge on, allowing for observation of the spiral structure. A weak bar may be present through the center of the bulge. Star formation is occurring within the galaxy and at moderate levels based on the coloration in the spiral arms.
