The observed galaxy presents as a relatively compact object. It appears to have a somewhat diffuse morphology without a clearly defined disk structure. The overall light distribution suggests a moderate level of central concentration, with the brightest region located near the apparent center.

The color indices inferred from the available data suggest that the object exhibits a bluer spectral energy distribution in its central region. There is also evidence of a more extended, redder component surrounding the central region. This could indicate ongoing star formation in the central region, or the presence of a young stellar population.

The galaxy shows possible signs of minor disturbances in its overall shape, however, these are not substantial. It could be that the galaxy is involved in a minor merger or interaction with a smaller companion galaxy. However, the possibility of a chance alignment with another background object can not be excluded. 