The galaxy presents as a somewhat elongated, likely disc-shaped structure, oriented at an angle to our line of sight. The central region exhibits a higher concentration of light, suggesting the presence of a bulge. The galaxy displays a relatively smooth texture, hinting at a lack of prominent spiral arms. There is a color gradient from the central region to the outer edges, transitioning from a yellow-orange hue in the core to a slightly bluer tone in the surrounding disk. This gradient implies a difference in stellar populations, with older, redder stars likely dominating the bulge and a younger, bluer population present in the disk. The overall morphology suggests a galaxy that may be undergoing a relatively low rate of star formation, with a mass within the typical range for galaxies of this type. There are no apparent signs of major mergers or tidal disturbances in this image, although a minor interaction cannot be ruled out. The galaxy appears to be relatively isolated in its immediate vicinity.
