The galaxy exhibits a generally elliptical morphology, appearing mostly smooth with a high degree of central concentration. The light distribution is relatively uniform with no discernible spiral arm structures or dust lanes. The color profile suggests the presence of an older stellar population, although a subtle blue tinge indicates some level of recent or ongoing star formation. The galaxy does not appear to be undergoing any major mergers or strong tidal interactions. The galaxy appears to be generally round with a smooth profile. 
