The galaxy presents as a slightly inclined disk galaxy, potentially of type spiral or lenticular. The central bulge exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the center, a faint and diffuse disk is visible, with a subtle bluing of color. This may be indicative of regions of more recent star formation within the disk. There is no clear indication of strong spiral arm structure. The overall smoothness of the light distribution suggests a relatively evolved system, with a possible lack of ongoing major mergers or interactions. The galaxy does not present obvious signs of significant disturbance or active galactic nucleus activity, based solely on the visible morphology and color distribution.
