The observed galaxy presents an elongated, cigar-shaped morphology, suggestive of an elliptical galaxy viewed at an oblique angle, or potentially a spiral galaxy seen edge-on. The central region exhibits a bright, concentrated luminosity, indicative of a dense stellar population, possibly an older population given the color. This suggests that star formation may be relatively low. The galaxy's color profile trends towards redder hues, implying a population dominated by older, redder stars and/or significant dust obscuration. There are no readily apparent features such as spiral arms or prominent dust lanes. Given its apparent smoothness, there is no indication of any major recent mergers. Slight irregularities could indicate minor disturbances.
