The galaxy appears as a concentrated central bulge surrounded by a less defined, somewhat diffuse disk. The color profile reveals a yellowish core, suggestive of an older stellar population. There's a subtle hint of bluer hues in the outer regions of the disk, potentially indicating ongoing star formation, although this is not strongly pronounced.

The galaxy's shape seems to deviate slightly from being perfectly round, tending towards an elliptical form. There are indications of a minor disruption, with some asymmetric features that could be attributed to past interactions or internal dynamical processes. No strong signs of tidal tails or major mergers are evident.

The overall morphology suggests a galaxy in transition, possibly an early-type spiral or a lenticular galaxy with a modest amount of recent star formation in its disk.
