The galaxy presents a generally smooth morphology, appearing largely featureless in this imaging. Its overall shape is elliptical, with a high degree of roundness. The color profile suggests an evolved stellar population, with the central region exhibiting a yellow-orange hue, indicative of older, redder stars. There is minimal evidence of active star formation as judged by a lack of bright blue regions typically associated with young, hot stars. There may be some minor tidal disturbances present. The galaxy doesn't seem to have any merging activity with other galaxies. The galaxy's size appears relatively small in angular extent, implying a substantial distance.
