The galaxy presents as a relatively smooth, centrally concentrated object, with a high degree of roundness in its overall morphology. There is minimal evidence of distinct spiral arm structures or prominent features such as dust lanes or star-forming regions. The galaxy appears to be dominated by a bright central bulge, with a more diffuse halo surrounding it. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although some subtle irregularities may be present. Color gradients appear to be subtle, with a generally consistent yellowish-white hue across the visible extent of the galaxy. The galaxy is a medium-sized galaxy with moderate star-forming activity, and most of the stars seem to be older stars.