The galaxy presents a generally smooth, elliptical morphology. The light is highly concentrated toward the center, exhibiting a bright, unresolved core which suggests the presence of an active galactic nucleus, or a very dense concentration of stars. The light then gradually diffuses outwards with no visible spiral arms, bars, or distinct features to disrupt the smooth morphology. The galaxy appears somewhat rounded, with only a very slight deviation towards an elongated shape. There's no strong evidence of tidal tails, merging companions, or other major disturbances in its structure, although there could be faint, minor irregularities. The color appears to be redder than blue suggesting a relatively older stellar population and reduced star formation.
