The observed galaxy presents as a spiral type. Its disk is clearly visible. The spiral arms appear to be well-defined, emanating from a central bulge. The winding of the spiral arms appears moderate. There is some evidence of a bar-like structure in the central region. The central bulge is of moderate size, neither overly dominant nor entirely absent. There are two main arms visibly coming out of the bulge. There does not appear to be signs of major interaction with another galaxy, though there is a slight asymmetry to the shape. The galaxy is neither completely smooth nor obviously irregular.
