The galaxy presents a largely smooth morphology, with a centrally concentrated bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Fainter, diffuse features extend outwards from the core, indicative of a disk, though it's relatively subtle. The overall shape is generally round, transitioning from elliptical closer to the core, to disk further out. There is no readily apparent evidence of ongoing major merger activity or significant tidal disturbances based on visible features, although there may be a very minor irregularity within the disk. Based on the color indices, the galaxy is likely experiencing low levels of star formation. The galaxy appears to be fairly massive.
