The galaxy presents as an elongated elliptical morphology. Its central region exhibits a concentrated luminosity, suggestive of a substantial stellar population. The galaxy displays a generally smooth texture, with no apparent spiral arm structures or distinct dust lanes visible. There is a slight asymmetry in its shape, potentially indicating a minor gravitational interaction. The color gradient transitions from a yellowish-white core towards a slightly bluer hue in the outer regions. Star formation appears to be present, even though the galaxy is largely characterized as a smooth, evolved system. Overall, the system seems to be a relatively massive galaxy undergoing a slow phase of star formation, with subtle indications of a recent or ongoing disturbance event.
