The galaxy presents an overall elliptical morphology with a smooth light distribution, suggesting characteristics of an early-type galaxy. Its core region appears quite bright and centrally concentrated, with a gradual decrease in luminosity toward the outer regions. There is only a slight suggestion of a disk, potentially indicating a low rotational velocity. The galaxy exhibits a weak reddish hue, potentially indicating an older stellar population or a higher concentration of dust attenuating the blue light. There are no apparent signs of recent or ongoing major mergers. A slight asymmetry is observed, but seems to be minor and may possibly be a weak tidal interaction.
