The galaxy presents as a moderately luminous, elongated structure. It appears to be a spiral galaxy viewed at a relatively high inclination. The central bulge is prominent, exhibiting a yellowish-white hue, suggesting an older stellar population. Faint spiral arms are observed extending from the bulge, with hints of bluer regions indicative of ongoing star formation. The overall color profile suggests a relatively low star formation rate. There is a possible minor companion galaxy nearby on one side. No significant signs of major mergers or strong tidal disturbances are observed within the limits of image resolution. The overall morphology seems relatively smooth and undisturbed.
