The galaxy presents a generally smooth morphology, with a somewhat elongated shape. The core is characterized by a concentrated, bright yellowish-white light, indicating a high density of older stellar populations or perhaps an active galactic nucleus. The light tapers off away from the core into what looks like a diffuse halo or disk. There may be a hint of faint spiral structure, but the smoothness is much more prominent. This is also supported by the lack of defined, blue star forming regions. Overall the galaxy seems to be in a more mature stage.

Based on the slight elongation and color profile, this galaxy could be an early-type spiral or lenticular galaxy, potentially transitioning from a more actively star-forming spiral to a passively evolving elliptical. Any signs of tidal disturbances are very minimal.
