The galaxy presents as a single, relatively smooth and consolidated object. Its morphology appears elliptical, with a notable lack of distinct spiral arms or a prominent disk structure. The light distribution is concentrated towards the center, indicating a bulge-dominated system. There's a slight elongation, suggesting that it isn't perfectly spherical. The dominant color is a yellowish-orange hue, suggestive of an older stellar population. There is little evidence of ongoing star formation, with no discernible blue or white regions associated with young, hot stars. The outer regions exhibit a gradual fading in intensity, lacking sharp boundaries. There may be minor disturbances or tidal features, but these are subtle and do not significantly disrupt the overall smooth appearance of the galaxy.
