The galaxy presents an elliptical morphology with a smooth light distribution, suggesting a lack of prominent spiral arms or a distinct disk structure. The central region exhibits a concentrated, bright core, potentially indicative of a supermassive black hole or a dense stellar population. The galaxy has a generally reddish color, which implies an older stellar population with fewer young, blue stars, and a low ongoing star formation rate. There appears to be some interaction or minor disturbance in the galaxy, possibly a minor merger event. A secondary, slightly fainter, area of light to the right of the central concentration implies that there is either some tidal effect or a faint second source in interaction.
