The galaxy appears as a slightly elongated, disk-like structure, viewed at an inclined angle relative to our line of sight. The central bulge presents a smooth, concentrated luminosity profile, exhibiting a yellowish hue, which suggests an older stellar population. Moving outwards from the core, a fainter, bluer disk becomes apparent. This color gradient potentially indicates ongoing star formation within the disk. However, based on the overall smooth appearance, prominent spiral arms are not evident, but a faint, unorganized disk is present. There are no obvious signs of tidal disturbances or a major merger event, suggesting a relatively quiescent state.
