The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular classification. It appears largely spheroidal, with a high degree of radial symmetry. The light profile exhibits a central concentration that gradually decreases outward. The color is relatively uniform across the galaxy, with a slightly redder hue. There is no obvious spiral arm structure or prominent dust lane visible. There is no clear indication of ongoing major merger activity or tidal disturbances. The light is concentrated within a diameter of approximately 7-8 kpc. This galaxy does not appear to exhibit a very high star formation rate.
