The galaxy appears to be an elliptical type, characterized by a smooth, relatively featureless morphology. It exhibits a centrally concentrated light distribution, appearing brightest towards the core. The overall shape is elongated, resembling a cigar shape, with the longest axis significantly greater than the shortest. The color profile suggests an older stellar population. The central region shows a yellowish hue, indicative of evolved stars, while the outer regions present a bluer tint. The structure exhibits no signs of significant ongoing mergers or tidal disturbances, suggesting a dynamically relaxed system. The galaxy does not appear to have prominent spiral arms or a well-defined disk structure. Overall, the appearance is consistent with an elliptical galaxy composed primarily of older stars with low levels of ongoing star formation.
