The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing somewhat elongated along a discernible axis. The light distribution suggests a prominent bulge component, which is indicated by the concentration of light in the central region. The color profile transitions from a redder core, likely indicative of an older stellar population, to bluer outer regions, suggesting ongoing or recent star formation. There are no obvious spiral arm structures or bar features. The galaxy appears to be a relatively isolated system, exhibiting no strong tidal features or signs of major interaction with other galaxies. The overall structure appears relatively undisturbed.
