The galaxy exhibits a generally elliptical morphology, appearing elongated rather than perfectly spherical. The light distribution suggests a relatively smooth profile with no prominent spiral arms or bar structures readily visible. The central region displays a bright, concentrated core, indicative of a high stellar density or possibly an active galactic nucleus. The overall color profile transitions from a yellowish-white core to a slightly redder hue in the outer regions. There may be some slight disturbances to the shape, but it is difficult to ascertain if they are due to interactions with another galaxy. The galaxy does not appear to be particularly dusty, as there is very little evidence of distinct dust lanes or patchy extinction. The general appearance suggests that the object is a relatively massive, evolved system.
