The galaxy presents as a single, relatively smooth object with a concentrated central bulge. There's a slight elongation to the structure, suggesting a possible, though not strongly defined, disk component, but overall, the shape leans toward elliptical. The color profile reveals a predominantly yellow to orange hue in the center, likely indicative of an older stellar population. The outer regions show hints of bluer tones, potentially signaling ongoing, albeit subdued, star formation. There's no clear indication of spiral arms or strong dust lanes. The galaxy doesn't exhibit any obvious signs of recent mergers or major disturbances, though a faint asymmetry cannot be entirely ruled out.
