The galaxy presents as a relatively compact structure, exhibiting a smooth, elliptical morphology. Its color profile indicates a dominant population of older stars, appearing predominantly yellow-orange. There is a subtle central concentration of light, suggesting a possible galactic nucleus. There is no evidence of spiral arms, dust lanes, or ongoing major merging activity. The galaxy's overall symmetrical shape suggests a dynamically relaxed system. Some faint features and disturbances may be present, but are obscured by the resolution. The galaxy appears to be relatively isolated, with no immediate signs of tidal interactions with neighboring galaxies.
