The galaxy presents a somewhat elliptical morphology. A prominent bulge is visible, exhibiting a yellowish hue suggestive of an older stellar population. Surrounding the bulge is a faint, bluish disk, indicating the presence of some younger, bluer stars and potentially ongoing star formation, though at a low rate. The galaxy's profile suggests it is viewed at an intermediate angle, not quite face-on nor edge-on. There is a slight asymmetry in the outer regions of the disk, potentially indicating a past minor interaction, or disturbance. The overall structure appears relatively smooth, with no major signs of disruption.
