The galaxy appears as an elliptical type, exhibiting a generally smooth and rounded morphology. There is a concentrated central bulge, which is the brightest part of the galaxy in this image. The light gradually fades as it extends outwards from the center. The overall color profile indicates a redder hue, implying a population of older stars and a lower rate of ongoing star formation. There are no apparent spiral arms or significant dust lanes visible. There are no signs of any major mergers or tidal disturbances present within the image. The shape is generally round, with only a very slight elongation.
