The galaxy presents a generally smooth and rounded morphology. Its light profile appears centrally concentrated with a gradual falloff in intensity moving outwards from the core. The central region exhibits a yellowish-white hue, indicative of an older stellar population. Fainter, more diffuse outer regions show hints of a bluer color, potentially suggesting the presence of younger, hotter stars or ongoing star formation at a low rate. No prominent spiral arms, bars, or other distinct features such as tidal tails or strong distortions are observed. The overall appearance suggests a galaxy that is not currently undergoing major merging activity. There are no distinct dust lanes visible.
