The galaxy presents as a centrally concentrated object with an elliptical morphology, showing a smooth and largely featureless profile. There is a slight elongation, but the galaxy is primarily rounded in appearance. The color profile is dominated by yellowish hues, suggesting a relatively older stellar population, and correspondingly suppressed levels of star formation. Faint blue regions may exist in the galaxy, indicating the presence of younger, hotter stars, but these are not very prominent. No distinct spiral arms, bars, or other major structural features are readily apparent. It appears that the galaxy is not currently undergoing any major mergers or tidal disturbances.
