The galaxy appears to be a luminous, relatively compact object, exhibiting a moderately elliptical morphology. A central bulge is clearly visible, possessing a bright, yellowish-white color, suggesting a population of older stars. A fainter, more diffuse disk surrounds the bulge, displaying a slightly bluer hue compared to the central region. This implies the presence of a younger stellar population and ongoing star formation within the disk. The overall light distribution appears relatively smooth, with only subtle indications of spiral arm structure or prominent dust lanes. There is a hint of some interaction/merging event that may be occuring with a very close companion.
