The galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population or possibly an active galactic nucleus, though further spectral analysis would be needed to confirm the latter. The overall color profile leans toward the redder end of the spectrum, implying an older stellar population with fewer young, hot stars. There is a subtle transition in color from the center to the outer regions, with the outer halo exhibiting slightly bluer hues compared to the yellow center. The shape is moderately elliptical. There appears to be a lack of distinct spiral arms or significant dust lanes, which would be expected in a spiral galaxy. There is no significant morphological disturbances or signs of a major merger event.
