The galaxy presents a moderately elliptical morphology, appearing somewhat flattened along its minor axis. The central bulge region exhibits a bright, concentrated luminosity, suggesting a high density of stars and potentially a supermassive black hole at its core. Surrounding the bulge, a fainter, more diffuse disk is visible, displaying a smoother texture than would be expected from a spiral galaxy, and the disk appears relatively uniform in color and brightness, hinting at a lack of prominent spiral arm structure. The observed light is redder overall, indicating a stellar population dominated by older, redder stars, which would be consistent with low levels of ongoing star formation. Faint dust lanes might be present within the disk, but the image resolution is too low to confirm their detailed structure. There are no clearly visible star-forming regions or HII regions within the galaxy, further suggesting a relatively passive evolutionary state.
