This galaxy presents as a relatively smooth, elliptical structure. Its central region exhibits a concentrated, bright core, indicative of a high stellar density or possible active galactic nucleus. The overall shape appears to be somewhat elongated, showing a slight cigar shape, and the luminosity fades gradually from the core outward, with no distinct spiral arms or prominent features visible. The galaxy’s color appears to be skewed towards the redder end of the spectrum, suggesting an older stellar population and a lower rate of ongoing star formation. There may be some minor disruption to its morphology, but it appears primarily undisturbed.
