This galaxy presents as a moderately bright, compact object. The core region exhibits a notably high surface brightness, appearing nearly saturated in this image. The morphology seems to be a largely spheroidal shape but is irregular. There is some degree of irregularity or faint tidal feature extending from the galaxy on one side. There is some asymmetry in the outer regions, suggesting potential past or ongoing interactions or disturbances. The galaxy displays a color gradient, with the central bulge appearing whiter, possibly indicating a population of older stars. The outer regions take on a bluer hue, likely due to the presence of younger stars and ongoing star formation. The lack of well-defined spiral arm structures implies that the classification may be an elliptical or lenticular galaxy, albeit with notable irregularities.
