The galaxy presents as a spiral galaxy with a moderate inclination relative to our line of sight. Its structure is characterized by a prominent central bulge exhibiting a yellowish hue, indicative of an older stellar population. Fainter spiral arms are visible extending from the central bulge. The arms appear somewhat tightly wound, but are not well defined; they appear less distinct. The blue/white color in the spiral arms suggests the presence of younger, hotter stars and active star formation regions. Overall, the galaxy appears relatively undisturbed. There are no obvious signs of a recent major merger event, such as tidal tails or strong morphological distortions.
