The galaxy presents a generally smooth morphology, appearing largely featureless across the observed wavelengths. Its overall shape is moderately elliptical, deviating slightly from a perfectly circular form. There is a noticeable concentration of luminosity towards the galactic center, indicating a significant bulge component. The color profile suggests a relatively old stellar population, with a redder hue dominating. Star formation appears to be relatively suppressed, given the lack of prominent blue regions typically associated with young, hot stars. There may be very minor disturbances suggesting a possible minor interaction with another object, though this could be from other reasons.
