The galaxy presents a relatively smooth, centrally concentrated morphology, exhibiting a slight elongation in its overall shape. The light distribution appears fairly uniform, with a gradual decline in intensity from the core outwards. There is no distinct spiral structure or bar visible in this image. Hints of internal structure may indicate mild disturbances. The galaxy appears to be of intermediate size. Its color profile suggests a mix of stellar populations. The galaxy does not appear to be actively merging with any other galaxies, though there is a possibility of minor tidal interactions.
