The galaxy appears to be a relatively smooth, elliptical type. Its central bulge is bright and concentrated, exhibiting a yellowish-orange hue, which suggests a population of older stars. Moving outwards from the core, the light fades gradually. There is little evidence of spiral arms or prominent dust lanes, implying a lack of significant ongoing star formation. The galaxy's overall shape is close to round, though a slight elongation is discernible. No major disturbances or interactions with other galaxies are visually apparent, although some minor asymmetries cannot be ruled out based on this image alone. The galaxy's color profile suggests a relatively passive stellar population with minimal recent star formation activity.
