The galaxy presents as a somewhat elongated structure, appearing as a flattened spheroid with an apparent cigar shape. The central region exhibits a brighter luminosity, suggesting a concentration of stars or potentially an active galactic nucleus, though the resolution limits definitive assessment. The color profile is dominated by bluer hues, indicating a stellar population with relatively young, hot stars, or possibly ongoing star formation activity. There's a subtle color gradient visible, with bluer regions potentially tracing spiral arm segments, though these are not clearly defined. The overall morphology appears relatively undisturbed, with no major signs of ongoing mergers or tidal interactions. The smooth, flattened shape suggests it may be an early-type spiral or lenticular galaxy.
