The galaxy presents as a moderately luminous object with an elliptical morphology. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or significant dust lanes. The central region exhibits a slight concentration of light, hinting at a possible galactic bulge or active galactic nucleus, though higher resolution imagery would be required for confirmation. The overall color is somewhat red-shifted with some yellow tones in the center, indicating a population of older stars and potentially lower rates of star formation. There appears to be a small, nearby companion galaxy possibly interacting with the central galaxy, displaying disturbed features that could be indicative of minor gravitational interaction or a previous merger event. Some visual artifacts are present, but do not seem to be significantly affecting the overall morphological assessment. The object does not appear to be undergoing a major merger at this time.
