The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. The light distribution suggests a centrally concentrated luminosity profile, typical of elliptical galaxies.  The galaxy appears generally uniform in color, displaying a yellowish hue indicating an older stellar population, suggesting reduced levels of current star formation. There are no apparent spiral arms or significant dust lanes visible.  There is no evidence of any active galactic nucleus or ongoing merger activity from visual inspection. The galaxy's light profile suggests that it could be a rather large and massive galaxy.