The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, appearing more in-between than distinctly round or cigar-shaped. There's a noticeable color gradient, shifting from a yellower core region to redder outer parts. No obvious spiral arm structure is discernible in this image. The galaxy does not appear to be undergoing a major merger event, or showing major disturbances, though subtle irregularities cannot be ruled out given the image's resolution. The light profile suggests an older stellar population is likely dominant, with relatively low ongoing star formation activity. 
