The galaxy presents as a somewhat elliptical structure, with a brighter, more concentrated central region suggestive of a bulge.  The color profile indicates a dominant older stellar population, particularly concentrated in the central bulge, with yellower hues.  Fainter, bluer regions extend outward from the central bulge, hinting at the presence of some younger stars and potentially ongoing, though subdued, star formation.  Evidence of minor disturbances is seen in the overall structure, as there is an irregular morphology, potentially indicative of a past or ongoing interaction or merger.  The galaxy does not appear to have well-defined spiral arms, suggesting that it is either an elliptical galaxy or a disturbed spiral.  It exhibits a relatively smooth overall appearance.  The approximate size is around 6 kpc in radius.
