The galaxy presents as an elongated, elliptical structure, with a smooth, diffuse appearance. The central region exhibits a higher concentration of light intensity, gradually decreasing towards the outer edges. The color profile appears to be generally uniform across the galaxy, with a slightly bluer hue indicating the presence of some younger stars, though the overall color suggests a population dominated by older stars. The galaxy does not exhibit any obvious spiral arm structure, suggesting it may be an elliptical or lenticular type galaxy. There is a faint extension of light from the center that makes the galaxy look nearly cigar-shaped, though the shape index suggests it is more rounded. There is some evidence of recent star formation, but not much, as the galaxy's estimated mass is not very large. The galaxy appears undisturbed, without any signs of ongoing major merger activity, though there may be evidence of minor tidal interactions from previous events.
