The galaxy presents as a spiral type, observed at a near edge-on inclination. A prominent central bulge is evident, appearing bright and somewhat diffuse. Two spiral arms are suggested by the light, winding loosely from the core. The galaxy displays an overall smooth appearance, with no substantial signs of major merging activity or strong disturbances. The dust lanes running through the arms and disk are indicative of ongoing star formation, supported by the galaxy's color and the concentration of light in the disk region. There is a suggestion of a bar feature running through the centre of the bulge.
