The galaxy presents an elongated morphology, with a discernible central bulge. The light distribution appears relatively smooth, suggesting a lack of significant spiral arm structure. The galaxy's color profile shifts from a bluer hue at the edges towards a redder central region. This color gradient may indicate ongoing star formation in the outer regions. The smoothness of the galaxy suggests an elliptical classification. There is a possible minor tidal tail, a faint extension of light emanating from the main body of the galaxy, suggesting recent or ongoing gravitational interaction. This distortion is subtle, suggesting that if there was a merger, it may have been a while ago.
