The galaxy presents an elongated, cigar-shaped morphology, suggestive of an elliptical type. The central region exhibits a concentration of light, appearing brighter and more yellow in color, possibly indicating an older stellar population. Fainter, bluish light is visible towards the outer edges, suggesting the presence of some younger, hotter stars. A hint of a disk-like structure may exist, though this is difficult to confirm without more detailed analysis. The overall structure appears relatively smooth, lacking prominent spiral arms or irregular features, but with some minor disturbances potentially indicating the presence of past or ongoing interactions or mergers. There is little evidence of significant ongoing star formation within the galaxy, suggesting a relatively passive state.
