The galaxy presents an overall smooth morphology, appearing as a somewhat elongated structure. The central region exhibits a bright, concentrated bulge of light, suggesting a high stellar density. The galaxy displays a subtle color gradient, transitioning from a yellowish hue at the core to slightly bluer tones in the outer regions. This could indicate the presence of younger stellar populations in the outskirts compared to the older stars in the center. There appears to be a hint of a disk-like structure, though it is not well-defined or prominent, giving the galaxy a lenticular-like appearance. There may be a small interaction with another object or internal disturbances visible; though, it may just be a normal tidal stream. The overall appearance suggests a galaxy with a moderately evolved stellar population and a relatively low current rate of star formation.
