The galaxy presents as an elliptical or spheroidal structure, appearing generally smooth and rounded in morphology. A concentrated central bulge is present, exhibiting a relatively uniform yellowish-orange color, indicative of an older stellar population. There is an absence of clearly defined spiral arms or significant dust lanes. The galaxy does not seem to display any major signs of ongoing merger activity or strong tidal disturbances, maintaining a relatively regular shape. The galaxy appears to be relatively compact.
