The galaxy appears to be relatively compact, exhibiting a dominant central bulge with a somewhat amorphous halo. The light profile suggests a centrally concentrated object, with a rapid decline in luminosity moving outward from the core. While there isn't a clearly defined spiral structure, there are some faint asymmetric extensions suggesting possible tidal interactions or minor disturbances. The galaxy's color is largely consistent throughout, presenting a cyan hue indicative of a population of intermediate to old stars. Additionally, there may be some indications of recent star formation activity.
