This galaxy presents a generally smooth and elliptical morphology. The central region exhibits a high degree of luminosity and appears yellowish-white, suggesting a concentration of older stellar populations. Moving outwards from the core, the color gradually shifts towards a more blue-green hue, indicative of younger stars or ongoing star formation, though the activity appears subdued. The galaxy’s shape is somewhat elongated, with an apparent cigar-like appearance. There is a faint suggestion of minor disturbance in its structure, possibly related to a past or ongoing interaction. Overall, this galaxy appears to be a massive system with a relatively low star formation rate.