This galaxy presents as a relatively smooth, centrally concentrated object. The light profile suggests a possible elliptical morphology, with the bulk of the luminosity emanating from the core region. The galaxy appears somewhat flattened rather than perfectly spherical. There is little evidence of significant dust lanes or spiral arm structures. The overall color of the galaxy appears to be skewed toward the redder end of the spectrum, suggesting an older stellar population and potentially reduced star formation. There might be a subtle, minor disturbance in the outer regions, but this is not distinct.
