The galaxy presents as a moderately inclined spiral, exhibiting both smooth and featured characteristics. The central bulge appears prominent, displaying a relatively smooth, concentrated luminosity. A faint disk is discernible, harboring subtle spiral arm structures. These arms are loosely wound, and exhibit slight irregularities, possibly indicating minor gravitational disturbances. The color gradient suggests a mix of stellar populations, with a tendency toward redder hues in the central bulge and bluer tones in the disk, characteristic of ongoing star formation activity within the spiral arms, albeit at a low rate. There appears to be a companion galaxy nearby, possibly suggesting a merger in process.
