The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth light distribution without prominent spiral arms or a strong central bar. The overall shape is elongated, with the major axis significantly exceeding the minor axis, suggesting a non-spherical morphology and some degree of flattening. The core region displays a higher concentration of light, indicating a central bulge or nucleus. While generally smooth, there might be faint indications of a disk-like structure extending outwards from the bulge region. There is no clear evidence of active star formation regions or significant dust lanes, and the galaxy appears relatively undisturbed, without major signs of mergers or tidal interactions. There may be minor disturbances visible within the galaxy. The color index (based on provided magnitudes) suggests a relatively older stellar population with a lack of intense blue light from young, hot stars.
