The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears close to elliptical, although not perfectly circular, exhibiting a slight elongation. The central region shows a high degree of luminosity, indicative of a dense stellar population and/or active galactic nucleus activity, but it is difficult to tell from this image. The color profile transitions from a bluer hue towards the outer edges, implying a younger stellar population within the spiral arms or disk, to a redder color towards the center, indicating an older stellar population with less active star formation. There is little evidence of distinct spiral arm structures or prominent dust lanes, suggesting this galaxy is relatively evolved or is currently undergoing a quiescent phase of star formation. No evidence of major mergers or tidal disturbances are immediately apparent, suggesting that the galaxy has been relatively undisturbed.
