The galaxy presents as a relatively smooth object with a concentrated central bulge. The overall shape appears elliptical, though not perfectly so, exhibiting a slight deviation from a perfect circle. The light distribution is centrally concentrated.

There is a subtle color gradient visible, with the core exhibiting a yellowish hue, indicative of an older stellar population. Fainter blueish regions extend outwards from the core, suggesting the presence of younger stars or regions of active star formation. There is some evidence of minor morphological disturbances, suggesting that the galaxy may have undergone past interactions with another galaxy. The presence of these potential disturbances suggests that the galaxy may be in a period of evolution, perhaps a merger in progress.
