The galaxy presents as a moderately luminous, elongated structure. It appears to be a spiral galaxy of intermediate size, with a noticeable disk component. The morphology suggests a degree of disturbance or interaction. A prominent central bulge is evident, with a concentrated, bright core. The spiral arms are not well-defined, but hints of a disrupted arm structure suggest a possible minor merger or tidal interaction. There is a presence of star formation within the galaxy. The color of the galaxy is predominantly yellow, with areas of red, potentially indicating older stellar populations. The appearance of the galaxy's shape also suggests that the central areas are a smooth component, but some irregularities are apparent which might be caused by faint disk features. Overall, this galaxy's morphology points towards a system undergoing some form of gravitational interaction, evidenced by the disrupted arm features and possible merger activity.
