The galaxy presents as a relatively smooth, elliptical structure. It appears elongated, with a major axis roughly three times the length of its minor axis. The central region exhibits a high surface brightness, indicative of a concentrated stellar population or active galactic nucleus, however the image quality makes discerning the cause difficult. The color profile suggests a evolved stellar population, with a redder hue concentrated in the core, fading to slightly bluer tones in the outer regions. There is subtle morphological disturbance visible, possibly indicating a prior merger event or tidal interaction. The image resolution is insufficient to resolve individual stars or distinct spiral arm structures. The overall structure seems to be generally symmetric. There are some minor dust lanes visible, however they do not impact the structure significantly.
