The galaxy presents as a relatively compact object with a dominant central bulge. There is evidence of a faint, extended disk component. The color profile shifts from a yellow-orange hue at the core to a bluer tint in the outer regions of the disk. The morphology suggests a spiral galaxy, viewed at a slight angle relative to face-on. There is a subtle asymmetry visible which could indicate the presence of minor tidal disturbances, potentially from a past or ongoing interaction. Star formation is likely present, but appears at a relatively subdued rate, particularly within the central regions.
