The galaxy appears as a somewhat elliptical, smooth system with a bright central bulge and a fainter, extended halo. The core exhibits a yellowish-red hue, suggesting an older stellar population or significant dust obscuration. The outer regions of the galaxy show a bluer tint, potentially indicating ongoing star formation within a disk-like structure. No prominent spiral arms or bar structures are clearly visible. The overall morphology suggests that the galaxy may be in transition between a spiral and elliptical shape. There is a possible tidal disturbance occurring that is causing the disk to become more diffuse in appearance. There are some irregular features in the galaxy's outer regions that may suggest a recent merger or interaction with a smaller galaxy, but this is not apparent. The light is fairly uniform without apparent star forming regions.
