The galaxy presents as a spiral type. Two well-defined spiral arms are visible. These arms emanate from a moderately sized central bulge and exhibit a medium winding pattern. The bulge is primarily yellow, suggesting an older stellar population. The spiral arms display a bluer hue, possibly indicating the presence of younger, hotter stars and ongoing star formation. The galaxy is not edge-on, instead, it is at a slight angle. There is no evidence of any major merging or significant tidal disturbances within the galaxy's structure. The spiral arms extend to a noticeable but not extreme length, giving the galaxy a relatively compact but clearly structured form. There is evidence of a weak bar structure in the central region, as indicated by a slight elongation or distortion of the bulge. The galaxy's overall appearance suggests it is a relatively undisturbed and well-formed spiral galaxy undergoing normal star formation processes.
