The galaxy presents as a spiral type, exhibiting a distinct disk structure viewed at a moderate inclination. The arms are prominent, suggesting an active star formation environment, with medium winding. The central bulge is of moderate size, contributing significantly to the overall luminosity of the galaxy. A bar structure appears to bisect the central region. There are hints of potential disturbances in the outer regions of the disk. The spiral arms are moderately resolved, and there appear to be two main spiral arms. The galaxy exhibits a colour gradient, with a bluer disk and a yellower bulge. The morphology suggests that is in an isolated environment, with no immediate indication of a major merging event.