The galaxy presents an overall elliptical morphology. It exhibits a relatively smooth structure, lacking prominent spiral arms or significant dust lanes. The central region displays a concentrated brightness, indicative of a substantial galactic nucleus. The galaxy appears elongated, with an approximate axis ratio suggesting it may be an E4 or E5 galaxy on the Hubble sequence. The color profile reveals a generally redder hue, particularly pronounced toward the core, possibly implying an older stellar population and suppressed star formation activity. Faint blue hues extend from the core, possibly indicating areas of mild star formation. No signs of ongoing major mergers or significant tidal disturbances are readily apparent in this image, though minor irregularities cannot be ruled out.
