The galaxy presents as a relatively smooth, elliptical structure. There is a noticeable central bulge exhibiting a yellow-orange hue, suggesting an older stellar population. The outer regions appear more diffuse and display a subtle blue tint, possibly indicating the presence of some younger, hotter stars, albeit at a significantly lower star formation rate. The overall shape leans towards an elongated, cigar-like morphology, though it predominantly appears in between a rounded and cigar shape. No major disturbances or merging events are immediately apparent; however, subtle distortions might be present upon closer inspection. Overall, it appears to be a relatively isolated galaxy that is not undergoing major interaction.
