The galaxy presents as a single, dominant light source. Its morphology appears largely smooth, lacking any distinct spiral arms or bar-like structures. The overall shape is approximately elliptical, with the major and minor axes exhibiting only a slight difference. The color profile is dominated by redder hues, with a central concentration of golden light that fades gently toward the outer edges of the object. There is little evidence of significant dust lanes or ongoing, large-scale star formation activity from this image. There is a very slight hint of asymmetric disturbance in the profile, but the galaxy appears to be in a relatively stable and evolved state.
