The galaxy presents a generally smooth morphology, although subtle features are discernible. The central region is more luminous and exhibits a distinct orange-red hue, suggesting a population of older stars and a potentially significant dust component. Moving outwards from the core, the galaxy appears less defined with a more diffuse and bluish tint. There is no prominent spiral arm structure; the light seems to be generally spread throughout the galaxy. Its overall shape is elongated, with an axial ratio greater than 2:1, and there is some evidence of minor disturbances in its outer regions.
