The galaxy presents a clear disk-like morphology, appearing to be viewed at a slight angle, not perfectly edge-on. There is a discernible bulge component, which appears moderate in size, contributing significantly to the overall luminosity in the central region. Faint spiral arms are present but not very well-defined, extending outward from the bulge. A bar feature appears to be prominent, running through the bulge. There is no visual evidence of a major merger or significant tidal disturbance, but a slight asymmetry or minor irregularity might be present in the outer disk regions. The colour profile suggests a relatively evolved stellar population, with a yellower central bulge and a bluer disk component implying ongoing star formation.
