The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, diffuse light distribution across its structure. The central region presents a brighter, concentrated luminosity, suggesting a dense stellar population or potentially an active galactic nucleus, though no clear signs of AGN activity are readily apparent in the image. The galaxy displays a slightly elongated morphology, tending toward a flattened spheroid, with a subtle cigar shape. There's no evident spiral arm structure or significant dust lane obscuration within the visible spectrum. Based on the smooth features, the galaxy likely contains an older stellar population with a relatively low star formation rate and no major ongoing mergers or disturbances, indicating a dynamically relaxed system. The galaxy's color is generally yellowish, implying a lack of intense blue star formation regions and a dominance of older, redder stars.
