The galaxy appears to be an elliptical galaxy, potentially of type E4-E5 based on its apparent ellipticity. The light distribution is smooth and centrally concentrated, exhibiting a gradual decrease in brightness from the core outwards. There is no obvious spiral arm structure or dust lane visible. The central region presents a bright and somewhat blue-tinted appearance, possibly indicating a population of younger stars within the core. The outer regions display a redder hue, suggesting an older stellar population. There is no immediately apparent evidence of a major ongoing merger event, although subtle asymmetries may indicate minor tidal disturbances or recent accretion. The galaxy is relatively isolated, with no other immediately interacting galaxies apparent in the field.
