The galaxy presents as an inclined spiral, possibly of type Sa or Sb, viewed at a moderate angle. The central bulge appears prominent and spheroidal, exhibiting a yellowish-white color, which suggests a population of older stars. Fainter, bluer regions extend outwards from the bulge, suggestive of a disk component containing areas of ongoing star formation. Evidence of spiral arm structure is subtle, with some hints of dust lanes or flocculent arms extending from the central region. There appears to be some minor irregularity in the disc, but with a generally smooth morphology. Overall, it suggests a mature spiral galaxy with a stable, non-interacting environment.
