The galaxy presents as a relatively compact object with a centrally concentrated luminosity profile. Its overall morphology appears smooth, lacking prominent spiral arms or a well-defined disk structure. The color gradient suggests a population of older stars, particularly concentrated towards the center of the galaxy with a redder hue. There is a subtle indication of bluer colors towards the outer edges, potentially suggesting some ongoing, albeit subdued, star formation activity in these regions. The galaxy exhibits a generally rounded appearance, showing no obvious signs of major tidal disturbances or interactions with other galaxies. There might be very slight asymmetry, although further analysis is needed to determine if this is an intrinsic feature or an artifact of the image quality.
