The galaxy presents as a centrally concentrated, relatively smooth object, exhibiting a primarily elliptical morphology with a high degree of roundness. There is little evidence of a prominent disk structure or spiral arms, suggesting it is likely an early-type galaxy. The color profile indicates a redder central region grading to slightly bluer hues in the outer portions, which is consistent with ongoing, though perhaps subdued, star formation activity. There is no obvious indication of a major merger or significant tidal disturbances, though a minor disturbance cannot be entirely ruled out. Its apparent size is relatively compact, indicating a substantial distance. Overall, the galaxy appears to be a massive system with a modest amount of recent star formation.
