The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light profile appears to diminish gradually from the core outwards, showing a degree of roundness with only a minor elongation along one axis. The color gradient suggests a dominant population of older stars, with a yellowish-red hue concentrated toward the central region, likely indicating a lower rate of ongoing star formation within that area. The outer regions exhibit a bluer tint, potentially indicating a smaller population of younger stars. There is no evidence of spiral arms or significant dust lanes. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances.
