The galaxy presents a somewhat amorphous structure, with a dominant, centralized bulge exhibiting a yellowish-orange hue, indicating a population of older stars.  A fainter, bluish-white region is observed to the northwest of the central bulge. This suggests an area of more recent star formation activity. Overall, the galaxy lacks a well-defined spiral structure but there are subtle disturbances and irregularities in the galaxy's outer regions, possibly due to past or ongoing minor interactions.  The overall color gradient suggests a relatively evolved system with some ongoing star formation.
