The galaxy appears as a moderately sized, relatively smooth object with a slightly elongated shape. The light distribution is concentrated towards the center, displaying a faint, diffuse halo extending outwards.  There is some suggestion of subtle internal structure, but no prominent spiral arms or bar features are discernible. The galaxy's color appears somewhat redder overall, potentially indicating an older stellar population and a lower rate of recent star formation. There appears to be a slight disturbance to the structure of the galaxy, possibly a minor interaction with a nearby galaxy or residual effects from a past merger.
