The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology. The central region displays a yellowish-orange hue, potentially indicative of an older stellar population. Extending outwards from the core are fainter, diffuse regions of light which have hints of blue, suggesting the presence of some younger, hotter stars. The overall shape is elongated, resembling a cigar shape rather than a perfect sphere, although the center is more rounded. There are signs of potential disturbances in the overall structure, suggestive of past or ongoing minor interactions, though not as substantial as a major merger event. The galaxy does not have a well defined spiral structure.
