The galaxy presents as an elongated, elliptical structure. The central region exhibits a concentrated luminosity, appearing significantly brighter with a yellow-red hue, suggesting an older stellar population. The outer regions of the galaxy gradually fade into the background, showing a smoother texture with no distinct spiral arm structures visible. There is a slight blue tinge on the edges of the galaxy, indicating the presence of a small amount of star formation. The overall morphology suggests a galaxy undergoing relatively little active merging, with the dominant feature being its smooth, spheroidal light distribution.
