The galaxy presents a somewhat elongated, cigar-shaped morphology. Its light distribution appears relatively smooth with a high degree of central concentration, suggesting it could be an elliptical galaxy. There is a subtle hint of a possible disk-like structure or arm feature. The galaxy's color profile exhibits a reddish hue with a noticeable yellow tint toward the center, indicative of an older stellar population and potentially lower levels of ongoing star formation. There are no obvious signs of major mergers or significant tidal disturbances in the main galaxy. The shape implies that the galaxy is likely an older system with a lower star formation rate.
