The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, round morphology. There is a high degree of central concentration, with a bright, yellowish core that gradually fades into the surrounding galactic halo. No distinct spiral arms or significant dust lanes are visible. The galaxy appears largely undisturbed, with no strong evidence of ongoing major mergers or tidal interactions. There may be a very faint hint of some minor disturbance but it is not significant. The overall color profile suggests an older stellar population, consistent with a low star formation rate.
