The galaxy presents as a somewhat smooth, elongated structure. Its overall shape is closer to elliptical than spiral. The light distribution suggests a bulge-dominated morphology, with a brighter, more concentrated central region that fades gradually outwards. There is faint evidence of what could be tidal features or minor disturbances, potentially indicative of a past or ongoing interaction. Color gradients are subtle, with the central region appearing slightly redder than the outer edges. Star formation appears present but is likely at a low rate based on color profiles. The galaxy's light profile is generally even, with few distinct features.
