This galaxy appears to be an elliptical galaxy, characterized by its smooth, diffuse light distribution. There is a high degree of central concentration, with the light intensity gradually decreasing from the core outwards. The morphology suggests a relatively homogenous stellar population without significant dust lanes or spiral arm features. The galaxy exhibits a slightly elongated shape, tending towards an elliptical rather than perfectly circular form. Coloration indicates the presence of older stellar populations with low levels of recent star formation, though there is some indication of star formation. There is no indication of any major mergers or disturbances.