The galaxy presents as a singular, relatively smooth object, exhibiting a centralized concentration of luminosity. Its shape is largely circular, showing a gentle decline in light intensity from the core outwards. There is minimal discernible structure within the galaxy; no spiral arms, bars, or significant dust lanes are immediately apparent in this observation. Faint, diffuse color variations are present, hinting at some level of stellar population diversity. There are subtle, but noticeable, regions of reddish hue, potentially indicative of older stellar populations or areas obscured by dust. The general appearance suggests a system without recent major merger activity. There is little visual evidence of star formation regions, which may indicate that star formation may not be very active at this time. The absence of clear structural features implies that the galaxy is either viewed at a relatively large distance or is inherently an older system.
