The galaxy exhibits a generally smooth morphology, appearing largely featureless at this resolution. Its shape is elongated, approaching a cigar-like appearance. The color profile suggests a concentration of older stellar populations, with a yellow-red hue dominating the central bulge and a slightly bluer disk. There is no visible evidence of spiral arms or prominent dust lanes. The light is concentrated toward the center, suggesting a relatively high degree of central mass concentration. The galaxy appears to be isolated, with no obvious signs of tidal interactions or ongoing merger events. The overall structure suggests a disk galaxy seen at a moderate inclination, with its apparent shape deviating noticeably from a perfect circle.
