The galaxy presents as an elliptical system, exhibiting a smooth, centrally concentrated luminosity profile. There is no discernible spiral structure or prominent disk component evident within the resolution constraints of the image. The galaxy appears largely featureless, lacking distinct dust lanes, star-forming regions, or tidal features suggesting recent major merger events. The morphology of the galaxy is consistent with an early-type system, with an overall color profile dominated by longer wavelengths, suggestive of an older stellar population. There may be some minor disturbances around the galaxy which indicates there has been some sort of gravitational interaction.
