The galaxy exhibits a concentrated, smooth morphology, appearing largely featureless across the observed bands. The central region displays a pronounced luminosity gradient, suggestive of a significant stellar bulge. The galaxy's overall shape appears to be somewhere in between round and elliptical. There may be a small merging galaxy next to the central galaxy. The color profile shows a relatively red hue in the core, transitioning towards a slightly bluer tint in the outer regions, hinting at ongoing, albeit subdued, star formation activity within the galactic disk. The relatively smooth structure and dominant bulge imply a later-type classification, potentially an early-type spiral galaxy. The galaxy is at an approximate distance where one kiloparsec subtends an observable angular size, allowing for reasonable estimations of physical dimensions based on the image scale.
