The galaxy presents as a generally smooth, elliptical-like structure, with a concentrated central bulge. There is little evidence of spiral arms or a distinct disk. The light distribution is fairly uniform and concentrated, with no bright knots or regions of intense star formation readily apparent. The color profile suggests an older stellar population, dominated by redder wavelengths; yellow and orange hues are dominant in the central region, transitioning to less pronounced, redder colors toward the outer edges of the galaxy. There is some very faint blue light that could be indicative of low levels of ongoing star formation, however this may also be a result of image processing and not necessarily an indicator of young stars. The galaxy shows minimal signs of tidal disturbances or ongoing mergers, and no morphological characteristics indicate it is undergoing active interactions with other galaxies.
