The galaxy presents an elongated, cigar-shaped morphology, suggesting it is likely an elliptical galaxy. The central region exhibits a strong concentration of light, indicative of a dense stellar population and/or an active galactic nucleus. A gradual fading of luminosity is observed towards the outer edges of the galaxy, consistent with a decreasing stellar density. There is a slight asymmetry in the light distribution, with a faint extension or tidal feature visible on one side, possibly hinting at a minor gravitational interaction or a past merger event. Overall, the galaxy appears relatively smooth in texture, with little evidence of prominent spiral arms or dust lanes. The galaxy has a reddish hue, suggesting that it contains an older stellar population with a relatively low star formation rate. 
