The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, centrally concentrated light profile. It possesses a largely homogenous structure with no obvious spiral arms, rings, bars, or prominent dust lanes visible in the image. The color gradient is subtle, shifting from a slightly bluer hue towards the center to redder tones in the outer regions. This gradient is consistent with an older stellar population dominating the galaxy's mass, as indicated by the redder color. There are no prominent features indicating ongoing major mergers or significant tidal interactions. There is little star formation activity. There are no features suggesting a strong active galactic nucleus.
