The galaxy presents as a spiral galaxy, viewed at a relatively high inclination. There is evidence of spiral arm structure, although the angle makes precise characterization difficult. A central bulge is readily apparent, exhibiting a yellowish color, suggesting an older stellar population within. The disk component displays a bluer hue, indicative of younger stars and ongoing star formation. There is no obvious presence of a strong central bar. There does not appear to be any major merging or tidal disturbances. The galaxy exhibits a generally smooth, organized structure.
