The galaxy appears as a relatively smooth, elliptical-shaped object. Its core exhibits a concentrated brightness, with the overall light distribution being fairly even and lacking in significant internal structures such as spiral arms or prominent dust lanes. The color profile suggests an older stellar population, as evidenced by the predominantly yellowish-red hue, likely indicating a paucity of recent star formation. No major merging events or tidal disturbances are apparent; however, there might be some minor asymmetry in the outer regions.
