The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated towards the center, exhibiting a bright, moderately round core region. The light gradually decreases in intensity outwards from the core. There is only faint evidence of a disk component, with possibly an even fainter hint of spiral arms. The galaxy does not appear to be undergoing any major merging events or experiencing significant tidal disturbances. There may be only minor indications of disturbances. Based on the colors in the image, it appears to have a redder overall hue, suggesting a population of older stars and limited current star formation. The galaxy has a considerable mass, which could indicate that this is an older system.
