The galaxy presents as a centrally concentrated object with an overall elliptical morphology. It appears moderately bright, with a distinct core that is significantly brighter than the surrounding regions. The galaxy exhibits a somewhat smooth appearance, with a noticeable lack of well-defined spiral arms or distinct features. There may be some indication of a slight disturbance or minor irregularity in its structure, potentially indicative of a minor interaction or merging event. The color profile suggests a mix of stellar populations. The central region appears bluer, suggesting younger, hotter stars, while the outer regions exhibit a slightly redder hue, potentially indicating older stars or dust obscuration. The galaxy is relatively compact, spanning a small angular extent. The core of the galaxy is quite dense with a strong magnitude. A faint "halo" can be observed that is diffuse and lacks well-defined boundaries. The data indicates this galaxy to be non-merging.
